  We investigate the gravitational lensing scenario due to Schwarzschild-like
black hole surrounded by quintessence (Kiselev black hole). We work for the
special case of Kiselev black hole where we take the state parameter
$w_{q}=-\frac{2}{3}$. For the detailed derivation and analysis of the bending
angle involved in the deflection of light, we discuss three special cases of
Kiselev black hole: non-extreme, extreme and naked singularity. We also
calculate the approximate bending angle and compare it with exact bending
angle. We found the relation of bending angles in the decreasing order as:
naked singularity, extreme Kiselev black hole, non-extreme Kiselev black hole
and Schwarzschild black hole. In the weak field approximation, we compute the
position and total magnification of relativistic images as well.
