  A static spherically symmetric metric in Einstein-scalar-tensor gravity
theory with a scalar field potential $V[\phi]$ is non-singular for all real
values of the coordinates. It does not have a black hole event horizon and
there is no essential singularity at the origin of coordinates. The weak energy
condition $\rho_\phi > 0$ fails to be satisfied for $r\lesssim 1.3r_S$ (where
$r_S$ is the Schwarzschild radius) but the strong energy condition
$\rho_\phi+3p_\phi > 0$ is satisfied. The classical Einstein-scalar-tensor
solution is regular everywhere in spacetime without a black hole event horizon.
However, the violation of the weak energy condition may signal the need for
quantum physics anti-gravity as $r\to 0$. The non-singular static spherically
symmetric solution is stable against the addition of ordinary matter.
