In consider the domain of applicability of general relativity (GR), as
a classical theory of gravity, by considering its applications to a a
variety of settings of physical interest as well as its relationship
with real observations. We argue that, as it stands. GR is deficient w
hether it is treated as a microscopic or a macroscopic theory of gravi
ty. We briefly discuss some recent attempts at removing this shortcomi
ng through the construction of a macroscopic theory of gravity. We poi
nt our that such macroscopic extensions of GR are likely to be nonuniq
ue and involve non-Riemannian geometrical frame works.