The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with a bright core that gradually fades outwards. The shape appears slightly elongated, not perfectly circular. The color profile shows a bluer hue in the central region, possibly indicating a higher concentration of younger stars or ongoing star formation there. Fainter, reddish components are observed in the outer regions, potentially representing older stellar populations. There are no apparent spiral arms or prominent dust lanes. Overall, the galaxy appears to be a fairly massive, evolved system, with some evidence of recent or ongoing star formation activity.