The galaxy exhibits an overall elliptical morphology, appearing somewhat flattened. The light distribution is centrally concentrated, with a bright core region that gradually fades outwards. The color profile suggests a relatively uniform stellar population, with a slightly bluer hue throughout the galaxy and especially bright in the center. There appears to be little evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears relatively undisturbed, without major signs of tidal interactions or recent mergers, indicating a possible lack of recent star formation.
