The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light distribution. The central region appears bright and concentrated, gradually fading towards the outer edges, indicating a relatively high stellar density in the core. The galaxy does not appear to have prominent spiral arms or significant dust lanes. There are some slight features on the outskirts, but they are probably minor distortions due to possible past interactions with other galaxies. The galaxy has a noticeable red color suggesting an older stellar population dominated by redder, evolved stars, and a low rate of ongoing star formation.
