  Here, an accelerated phantom model for the late universe is explored, which
is free from future singularity. It is interseting to see that this model
exhibits strong curvature for all time in future, unlike models with `big-rip
singularity' showing high curvature near singularity time only. So, quantum
gravity effects grow dominant as time increases in the late universe too. More
importantly, it is demonstrated that that quantum corrections to FRW equations
lead to non-violation of `cosmic energy conditions' of general relativity,
which are violated for accelerating universe without these corrections.
