The galaxy presents as a relatively smooth, elliptical or lenticular structure with a concentrated central bulge. There is little evidence of spiral arms or significant disk features from this angle. The core exhibits a yellowish-white hue, which could indicate a population of older stars, potentially with ongoing moderate star formation. The outer regions appear slightly bluer, possibly indicating younger stellar populations or enhanced star formation in these areas, although the overall color profile suggests an older population. The galaxy exhibits an elongated shape, leaning closer to an elliptical morphology. There are no visible signs of significant interaction or major tidal disturbances, although very minor features cannot be ruled out. The apparent smoothness of the galaxy suggests a system that is not undergoing major merging events.
