The galaxy presents an elliptical morphology. The central region exhibits a high degree of brightness, suggesting a concentrated stellar population. The light gradually decreases from the center outwards in an even distribution.

The overall color appears somewhat red, potentially indicating an older stellar population. The galaxy shows no strong signs of spiral arms or active star formation regions in the visible spectrum. There may be evidence of a minor merger, or tidal interactions. The isophotes of the galaxy are elliptical, with the major axis having a noticeable tilt. The galaxy does not appear to be a perfect circle, but is elongated. There is no visible disk.
