  We study photon orbits within (1+2)-dimensional Einstein-power-Maxwell
non-linear electrodynamics assuming a static and circularly symmetric
background. An exact analytical solution to the null geodesic equations for
light rays is obtained in terms of the Weierstra{\ss} function. We investigate
in detail the impact of the photon energy, the electric charge of the black
hole, and the integration constant (initial condition) on the shape of the
orbits.
