The galaxy presents as a relatively smooth, elliptical-like structure. It appears centrally concentrated with a bright, yellowish core, suggestive of an older stellar population, potentially dominated by evolved red giant stars. The overall light distribution suggests a high degree of radial symmetry, with a gradual decrease in luminosity extending outwards from the core. There is minimal evidence of spiral arms or significant dust lanes. Faint extensions may be present, but their signal is weak. No prominent features indicative of ongoing major mergers are apparent, though minor disturbances cannot be ruled out.
