The galaxy presents as a somewhat elongated, elliptical form, appearing more cigar-shaped than circular. Its core is characterized by a bright, concentrated luminosity. The surrounding regions show a gradual decline in brightness moving outward from the central bulge. The galaxy exhibits a smooth appearance with minimal discernible structure. There is no indication of strong spiral arms or dust lanes. The overall color profile suggests a population of older stars, with redder hues dominating. There is no obvious sign of significant star formation activity in the surrounding areas, implying a relatively quiescent state. There's no indication of ongoing merging activity or major disturbances in its morphology.
