The galaxy presents as a relatively smooth, elliptical-like structure. Its color is predominantly yellow-orange, suggesting an older stellar population with minimal ongoing star formation. There are no prominent spiral arms or dust lanes visible. The galaxy is roughly circular in appearance, with only a slight hint of elongation. No signs of tidal disturbances or interactions with other galaxies are apparent, implying it is an isolated system or has settled into a stable configuration following any past mergers. The galaxy has a concentrated central region, which may indicate the presence of a supermassive black hole. Its overall morphology suggests it is a mature galaxy that has largely exhausted its gas supply.