  The expansion rate of `Intermediate inflation' lies between the exponential
and power law expansion but corresponding accelerated expansion does not start
at the onset of cosmological evolution. Present study of `Intermediate
inflation' reveals that it admits scaling solution and has got a natural exit
form it at a later epoch of cosmic evolution, leading to late time
acceleration. The corresponding scalar field responsible for such feature is
also found to be a tracker field for both gravity with canonical and some
non-canonical form of kinetic term. Thus the so called Intermediate inflation
should be considered as yet another dark energy model with asymptotic de-Sitter
expansion.
