The galaxy presents an elliptical morphology, with a smooth and concentrated light profile. The galaxy exhibits a prominent central bulge, characterized by a yellowish-white hue, which likely indicates a population of older, lower-mass stars. The outer regions appear to fade gradually into the background, displaying a slightly bluer color, suggesting the presence of some younger stars or ionized gas, though star formation activity appears to be relatively low. No distinct spiral arm structures are discernible. The overall shape appears somewhat elongated, but not significantly distorted, suggesting a relaxed state without major recent mergers, though there are slight asymmetries.
