The galaxy presents as an elliptical system, appearing somewhat flattened in shape. Its light profile shows a centrally concentrated, bright core region that gradually fades into a diffuse halo. The color distribution indicates an older stellar population, with a yellowish-red hue dominating the core. There is minimal evidence of active star formation, as indicated by the lack of prominent blue regions typically associated with young, hot stars. A smooth morphology is apparent, without any noticeable spiral arm structure or significant dust lanes. Some faint irregularities in the outer halo may suggest minor tidal interactions or past merger events, but this is uncertain given the image resolution. The galaxy is likely a relatively massive system, given its size and overall luminosity.
