  The present study reports a reconstruction scheme of a Dark Energy (DE) model
with higher order derivative of Hubble parameter, which is a particular case of
Nojiri-Odintsov holographic DE [S. Nojiri and S. D. Odintsov, Gen. Relativ.
Gravit. 38 (2006) 1285.] that unifies phantom inflation with the acceleration
of te universe on late-time. The reconstruction has been carried out in
presence of bulk-viscosity, where the bulk-viscous pressure has been taken as a
function of Hubble parameter. Ranges of cosmic time $t$ have been derived for
quintessence, cosmological constant and phantom behaviour of the equation of
state (EoS) parameter. In the viscous scenario, the reconstruction has been
carried out in an interacting and non-interacting situations and in both the
cases stability against small perturbations has been observed. Finally, the
slow roll parameters have been studied and a scope of exit from inflation has
been observed. Also, availability of quasi exponential expansion has been
demonstrated for interacting viscous scenario and a study through tensor to
scalar ratio has ensured consistency of the model with the observational bound
by Planck. Alongwith primordial fluctuations the interacting scenario has been
found to generate strong dissipative regime.
