  Inhomogeneous cosmological models such as the Stephani universes could, in
principle, provide an explanation for the observed accelerated expansion of the
Universe. Working with a concrete, popular model of the Stephani cosmology --
the Stephani-Dabrowski model, we found that it is entropically viable. We also
comment on the energy conditions and the two-sheeted geometry of the spacetime.
However, similar to the LTB models, despite satisfying the holographic
principle, Stephani cosmology has difficulty satisfying all the constraints
from observations.
