The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing somewhat elongated, suggesting it is likely an elliptical galaxy viewed at an angle. The color distribution is dominated by yellow and red hues, indicative of an older stellar population, with a possible lack of ongoing significant star formation activity. The central region is brighter and yellower than the outer regions. There is a slight asymmetry, indicating a potential minor disturbance or interaction with another galaxy, or possibly an internal dust lane. Based on these characteristics, this galaxy is likely a massive system with a substantial amount of older stars.
