The galaxy presents as a diffuse, centrally concentrated object. It exhibits a generally elliptical morphology, appearing somewhat rounded in shape. There is a slight asymmetry or possible tidal disturbance visible on the left side of the galaxy, suggesting potential interaction with a smaller object or past merger event. The color appears relatively uniform across the galaxy, tending toward bluer wavelengths, with an absence of prominent dust lanes or distinct spiral arm structures discernable at this resolution. The galaxy’s smooth appearance suggests a potential classification as an elliptical or S0 galaxy. There may be evidence of tidal tails, which suggests that a merger might be possible. 
