The galaxy exhibits a moderately luminous, elliptical morphology, presenting a smooth, relatively featureless appearance. Its overall shape is generally round with some indication of a slight elongation. A concentrated central bulge is apparent, displaying a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy appear fainter and bluer, potentially indicating the presence of some younger stars or ongoing star formation. There is a subtle hint of a disk component, though not sharply defined, with no clearly discernible spiral arms or bar structures. Minor disturbances or tidal features are absent, indicating no recent major mergers. Based on the colors and the presence of what seem to be younger stars, the galaxy is likely experiencing some level of star formation.
