  We examine the thermodynamic properties of inner and outer horizons in the
background of Ho\v{r}ava Lifshitz black hole. We compute the \emph{horizon
radii product, the surface area product, the entropy product, the surface
temperature product, the Komar energy product and the specific heat product}
for both the horizons of said black hole. We show that surface area product,
entropy product and irreducible mass product are \emph{universal} quantities,
whereas the surface temperature product, Komar energy product and specific heat
product are \emph{not universal} quantities because they all are depends on
mass parameter. We also observe that the \emph{First law} of black hole
thermodynamics and \emph {Smarr-Gibbs-Duhem } relations do not hold for this
black hole. The underlying reason behind this failure due to the scale
invariance of the coupling constant. We further derive the \emph{Smarr mass
formula} and \emph{Christodolou-Ruffini mass formula} for such black hole
spacetime. Moreover we study the stability of such black hole by computing the
specific heat for both the horizons. It has been observed that under certain
condition the black hole possesses second order phase transition.
