The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that gradually fades into an extended halo. The light distribution suggests a lack of prominent spiral arms or distinct features typically associated with disk galaxies. There may be a slight elongation, but the overall shape is generally rounded, not obviously disturbed or undergoing a major merging event. Its color is somewhat yellow-shifted, suggestive of a population of older stars. The galaxy's features are relatively uniform, lacking significant internal structure. The light is smoothly distributed, with a gradual decrease in intensity moving from the center outwards. No apparent dust lanes or significant patches of star formation can be observed in the image.
