The galaxy presents an elliptical morphology, although not perfectly spherical; its shape is more akin to being in between round and cigar-shaped. The color profile suggests a significant population of older stars, with a yellowish-orange hue dominating the central region, transitioning to a slightly bluer hue towards what may be an outer disk. There is some indication of minor gravitational disturbance, possibly a small tidal tail or asymmetry. While the bulk of the galaxy is smooth in appearance, close inspection reveals some faint signs of possible disk or spiral structure.