  In this paper, we study some relevant cosmological features of a Dark Energy
(DE) model with Granda-Oliveiros cut-off, which is just a specific case of
Nojiri-Odintsov holographic DE unifying phantom inflation with late-time
acceleration, in the framework of Chameleon Brans-Dicke (BD) Cosmology.
Choosing a particular ansatz for some of the quantities involved, we derive the
expressions of some important cosmological quantities, like the Equation of
State (EoS) parameter of DE $w_D$, the effective EoS parameter $w_{eff}$, the
pressure of DE $p_D$ and the deceleration parameter $q$. Moreover, we study the
behavior of statefinder parameters $r$ and $s$, of the cosmographic parameters
$j$, $s_{cosmo}$, $l$ and $m$ and of the squared speed of the sound $v_s^2$ for
both case corresponding to non interacting and interacting Dark Sectors. We
also plot the quantities we have derived and we calculate their values for
$t\rightarrow 0$ (i.e. for the beginning of the Universe history), for
$t\rightarrow \infty$ (i.e. for far future) and for the present time, indicated
with $t_0$. The EoS parameters have been tested against various observational
values available in the literature.
