The galaxy presents as a centrally concentrated, smooth elliptical morphology. It exhibits a dominant spheroidal component with a high degree of radial symmetry. The core is a bright yellow, suggesting a large population of older stars. The outer regions fade gradually into the background, demonstrating a lack of distinct spiral arm structure or prominent dust lanes. There is a very faint, tenuous halo visible, extending slightly further along one axis, hinting at a possible minor interaction or past merger event, though the overall structure remains largely undisturbed. Color gradients suggest an increasing age of stellar populations towards the galactic center.
