The galaxy appears to be a relatively smooth, elliptical system. It presents a slightly elongated morphology but overall is not far from being circular in shape. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a population of older stars, leaning towards the redder end of the spectrum, with some contribution from younger, bluer stars. There are slight indications of a minor disturbance, such as a faint tidal feature or asymmetrical light distribution, which could be indicative of a past or ongoing minor merger event. No major mergers are apparent. The overall impression is that of a massive galaxy with ongoing star formation.
