  Starting from an inhomogeneous space-time model of the universe we could
recreate a scenario of recent time accelerating universe dominated by Dark
Energy type of fluid. The background matter component of such a universe was
considered to be made up of a combination of an anisotropic fluid, a barotropic
fluid and the presureless cold dark matter. It was found that inhomogeneity
exhibits itself as the curvature term in such a universe. We corroborated our
model with recent supernova Ia-JLA data together with $H_{0}$ data and BAO
data. Cosmographic analysis of the dynamical variables further show that the
model can mimic the $\Lambda$CDM cosmology very closely.
