The galaxy presents as a relatively smooth, elliptical morphology. Its light profile is concentrated toward the center, exhibiting a bright, yellowish core. The isophotes appear largely regular, with a gradual decrease in intensity moving outward from the nucleus. There is a very faint suggestion of a slight flattening or elongation, but no discernible spiral arms or bar structures are evident. The galaxy's overall color suggests a population of older stars, with only subtle hints of bluer regions, possibly indicating areas of ongoing, albeit limited, star formation. There do not appear to be any signs of major tidal disturbances or ongoing mergers.
