In this paper, we deal with spatially homogeneous and anisotropic Bianchi types-IX and Universe filled with Holographic dark energy and cold dark matter. Assuming the condition that the shear scalar is proportional to expansion scalar, we have obtained solutions of Einstein field equations. The Statefinder diagnostic pair i.e. {r‚s} is adopted to distinguish our dark energy models from other dark energy models. Some important physical features of the models have been discussed.