The galaxy presents a primarily smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, yellow-white core. The overall shape appears largely round, deviating minimally from perfect circularity. There are no readily discernible spiral arm structures or significant dust lane features. Faint blue-ish tinges may indicate pockets of star formation. Indications of a past merger can not be ruled out, but the galaxy has a relaxed, unperturbed appearance. Overall, a low star formation rate is likely.
