The galaxy presents a largely smooth, elliptical morphology. It displays a concentrated central bulge, with a gradual decline in luminosity outward from the core. The light profile suggests minimal presence of spiral arms or distinct disk structures. The galaxy exhibits a yellowish-white color, indicative of an older stellar population. There is little evidence of significant dust lanes or active star formation regions within the observable structure. The overall appearance is consistent with an early-type galaxy, potentially classified as an elliptical or S0 galaxy. The galaxy is relatively isolated, with no immediately apparent signs of tidal interactions or recent mergers.
