The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a reddish-orange hue suggestive of an older stellar population and diminished star formation activity. The surrounding halo shows a more diffuse, yellowish color, possibly indicating a mix of older stars and some ongoing, albeit low-level, star formation. The overall shape is moderately elliptical, deviating slightly from perfectly spherical symmetry. There is a possible indication of a minor gravitational disturbance.
