  In recent times, there has been an increasing interest with theories of
modified gravity as a means to gain a deeper understanding of the universe's
late-time acceleration phase. In this study we focused our attention on a
specific cosmologically viable $f(R)$ model. We performed a dynamic stability
analysis of this model, revealing that the model supports presence of just one
asymptotically stable solution which can explain the present-day acceleration
of the universe.
