The galaxy presents as a predominantly smooth, elliptical structure with a concentrated, bright central bulge that appears yellowish-orange in color. The galaxy appears relatively isolated with no immediately apparent major disturbances or merger events. The shape is neither perfectly round nor highly elongated, appearing moderately elliptical. There are no spiral arms or dust lanes visible, suggesting that this is most likely a massive elliptical galaxy with very low star formation. The galaxy's central region is significantly brighter than the surrounding halo, indicative of a higher stellar density towards the core. The lack of any visible structure beyond the smooth profile suggests an evolved system.
