The galaxy presents a somewhat elliptical morphology. Its color appears to be primarily yellowish-white, indicating a likely older stellar population. There is evidence of what appears to be a merging event, with a secondary structure or disrupted region visible within the galaxy's main body, suggesting a potential interaction with another galaxy. A significant portion of the galaxy seems to be smooth in texture, however there are areas of distortion and elongation suggesting that it may not be a simple elliptical galaxy. The galaxy exhibits a centrally concentrated region which implies a high density of stars or perhaps a supermassive black hole.
