The galaxy exhibits a roughly elliptical morphology, appearing somewhat rounded in shape. The central region displays a concentrated luminosity, characterized by a yellowish-white hue, suggesting an older stellar population. The outer regions appear fainter, with a subtle bluish tint, possibly indicating the presence of some younger, hotter stars, although the overall star formation rate seems to be relatively low. There is no distinct spiral arm structure or bar visible. The galaxy appears relatively undisturbed, with no obvious signs of major merging activity, although there may be some minor tidal disturbances present. The galaxy presents a smooth appearance and seems to be relatively isolated within the observed field.
