The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. A subtle, diffuse halo surrounds the central region, fading into a bluish tint, potentially indicating the presence of younger stellar populations or ongoing star formation at the periphery. The galaxy is relatively compact in appearance, with a somewhat elliptical shape, appearing nearly round. There are no obvious signs of tidal tails, strong interactions, or a dominant disk structure, indicating a likely classification as an elliptical galaxy. It exhibits a small hint of a disturbance, possibly a minor interaction event. Overall, it appears to be a fairly isolated, evolved galaxy.
