The galaxy presents a largely smooth, elliptical morphology. It exhibits a central bulge that appears bright and concentrated, transitioning outward into a more diffuse halo. There is no immediately apparent spiral structure or prominent disk. The galaxy's color gradient suggests a population of older stars dominating the overall light output, with a slight reddening towards the core. There's a notable absence of dust lanes or significant star formation regions, indicating a relatively quiescent state. The overall appearance is consistent with an early-type galaxy, likely an elliptical. A slight asymmetry in the outer halo suggests a possible minor interaction or past merger event.
