  The dynamical features of Bianchi type $VI_h$ $(BVI_h)$ universe are
investigated in $f(R,T)$ theory of gravity. The field equations and the
physical properties of the model are derived considering a power law expansion
of the universe. The effect of anisotropy on the dynamics of the universe as
well on the energy conditions are studied. The assumed anisotropy of the model
is found to have substantial effects on the energy condition and dynamical
parameters.
