There are hints of diffuse plumes beyond the jets emerging from the central galaxy (which does not seem to house a radio core, making this a #doublelobe ). If these plumes are genuine and not background noise, this could be quite a large source but because they do not generate a contour, I'm not comfortable labelling it as a potential giant candidate without confirmation from NVSS.
The bright compact source of radio emission near the edge of the image at about the 2 o'clock position seems unrelated and could be an #ifrs candidate.
by DocR scientist
nvss looks like the emission is pretty confined within a couple of arcmin. i agree, off to east (2 o'clock) looks unrelated.