  Upon applying Chamseddine's noncommutative deformation of gravity we obtain
the leading order noncommutative corrections to the Robertson-Walker metric
tensor. We get an isotropic inhomogeneous metric tensor for a certain choice of
the noncommutativity parameters. Moreover, the singularity of the commutative
metric at $t=0$ is replaced by a more involved space-time structure in the
noncommutative theory. In a toy model we construct a scenario where there is no
singularity at $t=0$ at leading order in the noncommutativity parameter.
Although singularities may still be present for nonzero $t$, they need not be
the source of all time-like geodesics and the result resembles a bouncing
cosmology.
