  In this study, we explore the mimetic matter model proposed by Chamseddine
and Mukhanov (J. High Energy Phys. 11, 135, 2013), utilizing the holographic
principle to coherently describe both the early and late universe when bulk
viscosity is present in the inhomogeneous equation of state. Our examination of
the universe's evolution is based on the generalized infrared-cutoff
holographic dark energy model detailed by Nojiri and Odintsov (Eur. Phys. J. C
77, 528, 2017) within the context of the flat FRW model. From a holographic
perspective, we derive the energy conservation equation incorporating mimetic
matter through a viscous holographic fluid model. Furthermore, we analyze
various scenarios of bulk viscosity by assuming a constant equation of state
parameter and derive the infrared cut-off expression in terms of the particle
horizon. We demonstrate that within the framework of mimetic gravity, there is
a class of solutions comparable to those in General Relativity, with an
additional contribution from a non-relativistic mimetic matter component. These
solutions can effectively describe dark matte
