The galaxy presents a roughly elliptical morphology, appearing significantly elongated. The central region exhibits a high surface brightness, with a concentrated core that dominates the overall luminosity profile. There is a notable color gradient observable within the galaxy, with the central region displaying a bluer hue, potentially indicative of ongoing or recent star formation activity. The outer regions of the galaxy exhibit a redder color. Faint asymmetric extensions or tidal features may be present, but these are subtle. Overall, the galaxy appears to be relatively isolated.
