The galaxy appears as an elliptical structure with a smooth, diffuse light distribution. It exhibits a slightly elongated shape but leans towards being more rounded. The galaxy's core presents a brighter, more concentrated luminosity, gradually fading outwards. There are no strong signs of spiral arm structure or significant dust lane obscuration visible in this image. Based on the color, it seems to be comprised of an older stellar population. No tidal tails or obvious signs of recent major merger events are seen, although there is a possible minor disturbance indicated. There may be another object that is interacting with the galaxy.
