The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. Its core appears bright, exhibiting a yellowish-orange hue, indicating a population of older stars. The surrounding halo is more diffuse and subtly tinged with green, suggesting the presence of some ongoing, though likely low-level, star formation. There are no readily discernible spiral arm structures or prominent dust lanes. The galaxy's overall form indicates it is likely in a relatively late stage of its evolution. It appears largely undisturbed, showing no signs of major mergers or tidal disruptions.
