The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions to a more diffuse halo. The core region appears yellowish, indicative of an older stellar population. The outer regions of the galaxy appear bluer, suggesting the presence of younger stars. No distinct spiral arm structures or significant dust lanes are visible. There are no apparent signs of a major merger event. A very slight distortion may indicate some minor gravitational interaction. The object's apparent size suggests it is a relatively large galaxy. Overall, the galaxy appears to be a mature system undergoing relatively little star formation.
