The galaxy presents as an elliptical morphology. The central bulge is a bright, concentrated yellow color, indicating a population of older stars. Moving outward from the core, the light gradually fades into a less defined disk. This is likely due to a lower density of stars and possibly some dust obscuration. There appears to be little to no prominent spiral structure or active star formation regions visible, consistent with it being classified as a fairly smooth system. There is little evidence of interaction or disruption in the image. It exhibits a shape that is somewhere between round and elongated.
