The galaxy appears as a largely homogenous, elliptical structure. It exhibits a dominant, smooth light profile concentrated towards its center, suggesting a spheroid-dominated morphology. The color gradient transitions from a yellow-orange core region to a more greenish-yellow outer halo, indicating potential variations in stellar populations or dust content with increasing radius. The overall round shape signifies a lack of significant rotational flattening and possible later type classification. There is little to no evidence of spiral arm structures, strong dust lanes, or irregular features within the galaxy, which further reinforces the classification as a possible elliptical galaxy with minimal ongoing star formation. The object has an approximate physical radius of 8 kpc and is likely a very massive galaxy.