The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is centrally peaked, indicative of a high concentration of stars toward the nucleus. The color appears somewhat redder in the core, suggesting an older stellar population. Fainter, bluer extensions surround the core, which may suggest a small presence of younger stars or potentially ongoing, low-level star formation. There is little evidence of strong spiral arm structure or significant dust lanes, pointing to a more evolved and less dynamically active system. The overall appearance implies that this is likely a massive galaxy that has largely completed its major star-forming phase. Slight disturbances are present in the outer regions, perhaps indicative of minor past or ongoing interactions or mergers.
