The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears elliptical, with a high degree of radial symmetry. There is no clear evidence of spiral arms or a distinct disk component. The light profile increases steadily toward the center, culminating in a bright, unresolved core. Subtle color variations are apparent, with the central region exhibiting a bluer hue suggestive of younger stellar populations, while the outer regions appear somewhat redder, potentially indicating older, more evolved stars. There is no indication of any major ongoing merger events.
