  In the present work, we have searched the existence of $\Lambda$CDM-type
cosmological model in anisotropic Heckmann-Schucking space-time. The matter
source that is responsible for the present acceleration of the universe consist
of cosmic fluid with $p = \omega\rho$, where $\omega$ is the equation of state
parameter. The Einstein's field equations have been solved explicitly under
some specific choice of parameters that isotropizes the model under
consideration. It has been found that the derived model is in good agreement
with recent SN Ia observations. Some physical aspects of the model has been
discussed in detail.
