  The paper considers a set of equations describing the static isotropic
gravity field of a macroscopic body within the framework of the theory of
gravity with a constraint. A general approximate solution of these equations is
obtained. The solution exists only at certain values for the three integration
constants. The out-of-body metric coincides with the Schwarzschild metric, but,
unlike the general relativity theory (GR), the curvature tensor invariants have
a certain finite value everywhere.
