  In this investigation we discuss the dynamical aspects of Kaluza-Klein FRW
type cosmological model in the presence of dark energy fluid and an attractive
massive scalar field. The field equations are solved using a power law between
the average scale factor and the scalar field to reduce the mathematical
complexity. We have presented the corresponding dark energy model. Important
cosmological parameters like equation of state (EoS) parameter, the
deceleration parameter, the density parameter and the jerk parameter are
evaluated. The physical behavior of the parameters is also discussed.
