The galaxy presents as a mostly smooth, elliptical morphology with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicating a significant population of older stars. A faint, diffuse halo of bluish light surrounds the central bulge, suggesting the presence of some younger stellar populations or ongoing, albeit low, levels of star formation. The overall shape is slightly elongated, appearing more "in between" round and cigar shaped, but without any obvious signs of significant spiral arm structures or major tidal disturbances. There may be some evidence of minor gravitational interactions, with some slight irregularities or asymmetries in the outer halo.
