The galaxy presents as a flattened, elliptical structure with a bright, concentrated central bulge. A diffuse disk surrounds the central bulge. The disk exhibits a somewhat smooth texture, lacking strong indications of well-defined spiral arms. The color profile suggests a relatively evolved stellar population, with a yellowish-white hue dominating the bulge region, indicating older stars. The disk appears slightly bluer than the bulge, hinting at the presence of some younger stellar populations or ongoing star formation, although the rate appears low. The galaxy shows no obvious signs of a major ongoing merger, although there is some indication of possible minor disturbances in the disk, suggesting the possibility of a minor interaction. The galaxy is inclined at an angle, with its major axis presented to the observer. The overall morphology appears consistent with a disk galaxy.
