The galaxy appears to be a relatively smooth, elliptical or lenticular system. It presents a centrally concentrated bulge that dominates its overall luminosity, appearing yellowish-white in color. The outer regions of the galaxy exhibit a more diffuse profile, with a subtle color gradient suggesting older stellar populations further from the core. There is a marginal indication of a disk component, but it is not clearly defined, contributing to the overall smooth, elliptical shape. There is no apparent dust lane or significant features to suggest recent or ongoing major merging events. The morphological classification leans toward a non-disturbed system.
