The galaxy presents as a relatively smooth, elliptical form. The central region exhibits a concentrated, bright, and yellowish-white core, suggesting a significant population of older stars. Moving outwards from the core, the light becomes less intense and shifts slightly towards bluer hues. There are minimal indications of spiral arms or other prominent disk-like structures. The galaxy appears moderately elongated. Some subtle disturbances are present, but it is not clear if they are mergers or other external phenomena. Overall, the galaxy appears to be a mature system, with a significant spheroidal component.
