The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting a population of older, evolved stars. The outer regions show a slightly bluer tint, which could indicate the presence of younger stars and ongoing star formation, although this is not a dominant feature. The galaxy is elongated, appearing more lens-shaped than perfectly spherical. There are no readily apparent signs of spiral arms or significant dust lanes. No tidal tails or other major disturbances are detected, which indicates a relatively isolated system without recent major merger events. A minor irregularity to the morphology of the disk is present on the lower edge, possibly the result of a minor disturbance. The overall appearance is consistent with an early-type galaxy.
