  The ambition of the present work is to highlight the phenomena of strong
gravitational lensing and deflection angle for the photons coupling with Weyl
tensor in a Kiselev black hole. Here, we have extended the prior work of Chen
and Jing \cite{1} for Schwarzschild black hole to Kiselev black hole. For this
purpose, the equation of motion for the photons coupled to Weyl tensor, null
geodesic and equation of photon sphere in a Kiselev black hole spacetime have
been formulated. It is found that the equation of motion of the photons depends
not only on the coupling between photon and Weyl tensor, but also on the
polarization direction of the photons. There is a critical value of the
coupling parameter $\alpha$ for existence of the marginally circular photon
orbit outside the event horizon, which depends on the parameters of black hole
and the polarization direction of photons. Further, the polarization directions
of coupled photon and the coupling parameter $\alpha$, both modify the features
of the photon sphere, the angle of deflection and the functions $(\bar{a}$ and
$\bar{b})$ for the strong gravitational lensing in Kiselev black hole
spacetime. In addition to this, the observable gravitational lensing quantities
and the shadows of the Kiselev black hole spacetime are presented in detail.
