  We have studied the locally rotationally symmetric (LRS) Bianchi type-I
cosmological model in $f(R,T)$ gravity ($R$ is the Ricci scalar and $T$ is the
trace of the stress energy tensor) with Bulk viscous fluid as matter content.
The model is constructed for the linear form $f(R,T)=R+2f(T)$. The exact
solution of field equations is obtained by using a time varying deceleration
parameter $q$ for a suitable choice of the function $f(T)$. In this work, the
bulk viscous pressure $\bar{p}$ is found to be negative and energy density
$\rho$ is found to be positive. The obtained model is anisotropic, accelerating
and compatible with the results of astronomical observations. Also, some
important features of physical parameters of this model have been discussed.
