The galaxy presents as a relatively bright and compact object. Its morphology appears largely elliptical, exhibiting a smooth, centralized distribution of light with minimal discernible internal structure or features such as spiral arms or a prominent bar. The galaxy exhibits a near-spherical profile, with a slight deviation towards being in between round and cigar shaped. The color profile suggests a population of older stars, indicated by the yellow-ish color, though it should be said that there may be some recent star formation. There is no evidence of a major ongoing merger or significant tidal disturbance, although there is a very slight probability of a minor disturbance.
