The galaxy presents an elliptical morphology, appearing as a somewhat flattened spheroid. Its color profile suggests a moderate population of older stars, with a concentration of light towards the redder end of the spectrum and a distinct yellowish hue. There is a noticeable central bulge that is bright and concentrated, which makes up a significant portion of the galaxy's overall luminosity. While the galaxy appears relatively smooth in structure, subtle irregularities and disturbances suggest the possibility of minor interactions or past mergers. There is no prominent disk-like structure or spiral arms visible. Overall, the galaxy presents a morphology indicative of a fairly evolved system, dominated by an aging stellar population.
