The object appears to be a relatively smooth, elliptical galaxy. It presents a centrally concentrated luminosity profile, with a bright core that gradually fades outwards. The galaxy exhibits a generally rounded shape, though there are subtle irregularities in its outer isophotes, possibly indicative of minor disturbances. The overall color of the galaxy is yellowish-orange, suggesting an older stellar population dominated by redder stars and a lack of significant recent star formation activity. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy seems relatively isolated, with no obvious signs of a major ongoing merger event. Faint hints of asymmetry might suggest past interactions or minor disturbances.
