The galaxy presents as a relatively smooth, elliptical structure, with a concentrated central bulge. There is a gradual decrease in luminosity from the core outwards, with no discernable spiral arms or prominent dust lanes visible in this image. The shape is elongated, somewhere in between round and cigar-shaped, indicating a possible classification as an elliptical galaxy. There do not appear to be any signs of major tidal disturbances or ongoing mergers. The galaxy exhibits a color gradient, appearing slightly bluer in the outer regions compared to the more yellow/orange central bulge, which may suggest some ongoing star formation, albeit at a modest rate, in the outer disk. Based on its red shift, the galaxy is relatively far away.
