  A detailed study of the various cosmological aspects in massive gravity
theory has been presented in the present work. For the homogeneous and
isotropic FLRW model, the deceleration parameter has been evaluated, and, it
has been examined whether there is any transition from deceleration to
acceleration in recent past, or not. With the proper choice of the free
parameters, it has been shown that the massive gravity theory is equivalent to
Einstein gravity with a modified Newtonian gravitational constant together with
a negative cosmological constant. Also, in this context, it has been examined
whether the emergent scenario is possible, or not, in massive gravity theory.
Finally, we have done a cosmographic analysis in massive gravity theory.
