After replacing the derivative in the Klein-Gordon equation with the minimal coupling prescription i.e. $\partial^\mu \to D^\mu \equiv \partial^\mu+ieA^\mu$. The equation becomes: \begin{equation*} ((\partial_\mu +ieA_\mu)(\partial^\mu+ieA^\mu)+m^2)\phi(x)=0 \end{equation*} \begin{equation*} (\partial_\mu\partial^\mu +m^2 +ie(\partial_\mu A^\mu +A_\mu \partial ^\mu)-e^2A_\mu A^\mu)\phi(x)=0 \end{equation*}
In the book "Introduction to Particle and Astroparticle Physics" by Alessandro De Angelis, the book makes the following substitution in the above equation calling it potential: \begin{equation} V(x)=ie(\partial_\mu A^\mu +A_\mu \partial ^\mu) \end{equation} which gives us the final equation. (neglecting $e^2$ term which is of second order): \begin{equation*} (\partial_\mu\partial^\mu +m^2 +V(x))\phi(x)=0 \end{equation*} My question is what is the significance of V(x)? As in what is this potential? Further if we assume the lorenz guage i.e. $\partial_\mu A^\mu =0$, how does that change the description of this potential?