$Ax^2+Bxy+Cy^2+Dx+Ey=-F$ General Form Conic
$$\frac{(x-h)^2}{a^2} + \frac{(y-k)^2}{b^2}=1 \tag{1} \label{1}$$ Standard elliptical form requires a "1" on the right side.
In this section we will work with the general form conic ellipse. Along the way we will show how to get a parametric equation from that general form.
The general form equation for a conic will permit it to be rotated within the plane such that the major axis is oriented at any angle to the $x$ axis. This Cartesian equation requires some linear algebra skills to be helpful. But there are a few things that we can discuss before that. The discriminant, $B^{2}-4AC$ is indicative of the conic shape. When the discriminant is less than zero then the shape will be elliptical, unless it is degenerate. The degenerate ellipse in elliptic form will be equal to zero. $$\frac{(x-h)^2}{a^2} + \frac{(y-k)^2}{b^2}=0 \tag{2} \label{2}$$ So long as the $xy$ term in the general form conic is zero, then you can transform the equation into elliptic form by completing the square in both $x$ and $y$. Having done so, if you get the form of $\eqref{2}$ and it is equal to zero then the ellipse is degenerate. $$B^{2}-4AC<0\qquad\text{Ellipse}$$ $$B^{2}-4AC=0\qquad\text{Parabola}$$ $$B^{2}-4AC>0\qquad\text{Hyperbola}$$
When the equation is graphed, it will be axis aligned if and only if $B=0$. If $B\ne0$, then there will be some amount of rotation.
All of the general equations written in variables $x$ and $y$ will reside in the $x,y$ plane. In order to get out of the plane (i.e. from $\mathbb{R}^{2}$ to $\mathbb{R}^{3}$), we have to use $$\begin{aligned} & \left(\begin{array}{c} x\\ y\\ z \end{array}\right)=\left(\begin{array}{c} CP_{x}\\ CP_{y}\\ CP_{z}\\ \end{array}\right)+a\cdot\cos(\theta)\cdot\mathbf{u}+b\cdot\sin(\theta)\cdot\mathbf{v}\\ & \qquad0\le\theta\le2\pi. \end{aligned}$$ which was discussed in the prior section. and we have to establish basis vectors in the new plane of interest. Since this section concerns equations in variables, $x$ and $y$, we will be in the standard $\mathbb{R}^{2}$ plane.
From the general form, obtain the two partial derivatives, set them to zero, and solve for $x$ and $y$ to get the center of the ellipse. This works whether or not the ellipse is rotated.
It is easy to translate the ellipse to the origin. For most everyone, that means pick up the ellipse and move it, without rotation, to have its center at $(0,0)$.
To do that, we write the ellipse as $$\begin{aligned} & A(x+h)^{2}+B(x+h)(y+k)\\ & +C(y+k)^{2}+D(x+h)\\ & +E(y+k)=-F \end{aligned}.$$ Notice that we have algebraically moved $F$ to the right hand side. If the algebra gets done correctly, then, when simplified, we will get a new set of coefficients and the terms in $x$ and $y$ will disappear.
The general form of an ellipse given by $Ax^{2}+Bxy+Cy^{2}+Dx+Ey+F=0$ can be written in matrix form as $$(x,y)\left(\begin{array}{cc} A & B/2\\ B/2 & C \end{array}\right)\left(\begin{array}{c} x\\ y \end{array}\right)+\left(D,E\right)\left(\begin{array}{c} x\\ y \end{array}\right)+F=0.$$ The $2\times2$ matrix has eigenvectors which when orthogonalized (i.e. made into unit vectors) constitute the basis vectors for the ellipse. Using the example ellipse, $8x^{2}+4xy+5y^{2}-42x-24y=-63$ $$Q\,:=\,\left(\begin{array}{cc} 8 & \frac{4}{2}\\ \frac{4}{2} & 5 \end{array}\right)$$ The eigenvalues come from the characteristic equation, we have $$(\lambda_{2},\lambda_{1})=\left(\begin{array}{cc} 8-\lambda & \frac{4}{2}\\ \frac{4}{2} & 5-\lambda \end{array}\right)=\lambda^{2}-13\lambda+36=0$$ $$\lambda_{1}=4\quad\lambda_{2}=9$$ To get the eigenvector, we write the vector equations: $$\left(\begin{array}{cc} 8 & 2\\ 2 & 5 \end{array}\right)\left(\begin{array}{c} x\\ y \end{array}\right)=\lambda_{1}\left(\begin{array}{c} x\\ y \end{array}\right)$$ and solve either one with $\lambda_{1}=4$. Using the top equation, $$8x+2y=4x$$ $$4x=-2y$$ $$2x=-y$$ let $x=1$,then $y=-2$ $$\mathbf{u}=\left(\begin{array}{c} 1\\ -2 \end{array}\right)\text{ matches with }\lambda=4$$ and with $\lambda_{2}$, I used the other vector equation here, but it does not matter. What matters is which eigenvalue is plugged in. $$2x+5y=9y$$ $$2x=4y$$ $$x=2y$$ let $x=2$, then $y=1$ $$\mathbf{v}=\left(\begin{array}{c} 2\\ 1 \end{array}\right)$$
These two vectors are graphed in figure 2 and a quick glance at the graph will show you that they align with the axes of the rotated ellipse. That could be useful.
There is one important thing to be done, and that is to normalize these eigenvectors. Otherwise, they will not serve a basis vectors in our parametric equation. $$\hat{\mathbf{u}}=\frac{\left(\begin{array}{c} 1\\ -2 \end{array}\right)}{\left\Vert \left(\begin{array}{c} 1\\ -2 \end{array}\right)\right\Vert }\qquad\qquad\hat{\mathbf{v}}=\frac{\left(\begin{array}{c} 2\\ 1 \end{array}\right)}{\left\Vert \left(\begin{array}{c} 2\\ 1 \end{array}\right)\right\Vert }$$ Putting some calculator numbers into all of this gets $$CenterP=\left(\begin{array}{c} 9/4\\ 3/2 \end{array}\right)$$ $$\hat{\mathbf{u}}=\left(\begin{array}{c} -0.8944\\ 0.4472 \end{array}\right)\qquad\qquad\hat{\mathbf{v}}=\left(\begin{array}{c} -0.4472\\ 0.8944 \end{array}\right)$$ and our parametrized equation can be written symbolically as $$\begin{aligned} & \left(\begin{array}{c} x\\ y \end{array}\right)=CenterP+a\cdot\cos(t)\cdot\hat{\mathbf{u}}+b\cdot sin(t)\cdot\hat{\mathbf{v}}\\ & 0 \le t\le2\pi. \end{aligned}$$ But we still haven't found values for $a$ and $b$. To get $a$ and $b$, we can set about to find the vertices. (Aside: $a=3/4$ and $b=1/2$.)One method to find the vertices is to rotate the ellipse into axes alignment. Since we know the eigenvectors, we can easily determine the rotation angle needed. It is $atan2(u_{y},u_{x})$ or $atan2(v_{y},v_{x})$ or $\arg(\mathbf{u)}$ or $\arg(\mathbf{v).}$ The results which differ by $\pi/2$, are $$\arg\left(\mathbf{u}\right)=2.0344\,rad=\theta_{1}$$ $$\arg(\mathbf{v})=0.4636\,rad=\theta_{2}$$ Our ellipse equation is $8x^{2}+4xy+5y^{2}-42x-24y=-63$, and the substitutions for rotation are $$\begin{array}{c} x=x_{1}\cos\theta-y_{1}\sin\theta\\ y=x_{1}\sin\theta+y_{1}\cos\theta \end{array}$$ which, after substituting and dropping the subscripts is $$\begin{aligned} & 8(x\cos\theta-y\sin\theta)^{2}\\ & +4(x\cos\theta-y\sin\theta)(x\sin\theta+y\cos\theta)\\ & +5(x\sin\theta+y\cos\theta)^{2}\\ & -42(x\cos\theta-y\sin\theta)\\ & -24(x\sin\theta+y\cos\theta)\\ & =-63 \end{aligned} $$ So that equation is oriented with the axes and after plugging in $\theta=2.0344\,rad$, we get $$4x^{2}+9y^{2}=\frac{9}{4}.$$ One easy way to find the vertices is to set $y=0$ and solve for $x$, and vice versa. $$\text{Horizontal Vertex}=\sqrt{\frac{9}{16}}=\frac{3}{4}=a$$ $$\text{Vertical Vertex} =\sqrt{\frac{1}{4}}=\frac{1}{2}=b$$ Now we can compute the vertices of the original ellipse using vector projection. $$\begin{aligned} & \left(\begin{array}{c} V_{1}\\ V_{2} \end{array}\right)=CP\pm a\hat{\mathbf{u}}\\ & =CP\pm a\left(\begin{array}{c} -0.8944\\ 0.4472 \end{array}\right)\\ & =\left(\begin{array}{c} 1.9146\\ 2.1708 \end{array}\right)\text{ and }\left(\begin{array}{c} 2.5854\\ 0.8292 \end{array}\right) \end{aligned} $$