  We study the interaction between dark energy (DE) and dark matter (DM) in the
scope of anisotropic bianchi type I space-time. First we derive the general
form of the dark energy equation of state parameter (EoS) in both
non-interacting and interacting cases and then we examine it's future by
applying a hyperbolic scale factor. It is shown that in non-interacting case,
depending on the value of the anisotropy parameter $K$, the dark energy EoS
parameter is varying from phantom to quintessence whereas in interacting case
EoS parameter vary in quintessence region. However, in both cases the dark
energy EoS parameter $\omega^{de}$, ultimately (i. e at $z=-1$) tends to the
cosmological constant ($\omega^{de}=-1$). Moreover, we fixed the cosmological
bound on the anisotropy parameter $K$ by using the recent observational data of
Hubble parameter.
