The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, unresolved core. The galaxy's light appears primarily uniform and relatively featureless, suggestive of an older stellar population. It has an elongated shape, rather than being perfectly circular. There is a slight hint of a disturbance or asymmetry in the outer regions, potentially indicating a minor gravitational interaction with a smaller companion galaxy. The overall color suggests that the galaxy has a lower star formation rate.
