The galaxy appears to be a luminous, elliptical system. It exhibits a smooth, centrally concentrated profile with a pronounced bulge. The central region displays a yellowish-orange hue, which may suggest an older stellar population. Fainter, diffuse light extends outward from the core, exhibiting a slight disk-like morphology. Subtle disturbances or asymmetries are noticeable in the outer regions. These may indicate recent or ongoing minor mergers.
