The galaxy presents as a generally smooth, elliptical morphology. It displays a prominent, concentrated central bulge with a yellowish-white hue, which suggests a population of older stars. Fainter, diffuse bluish-white structures extend from the central bulge, hinting at a disk-like component where some star formation may be present. The overall shape is somewhat elongated. There may be some evidence of a slight disturbance or interaction with a possible minor companion, but further investigation is required to confirm this. There is no obvious spiral structure or pronounced dust lanes visible.
