The galaxy presents as a centrally concentrated system with a generally elliptical morphology. The core appears quite bright and yellow-ish, indicative of an older stellar population. Moving outwards from the core, there is a gradual decrease in surface brightness. The inner regions exhibit a smoother texture. Some subtle faint blue extensions are observed in the outer regions, but overall the galaxy appears relatively undisturbed. The lack of significant dust lanes or prominent spiral arms supports a classification as a relatively smooth galaxy, possibly an elliptical or lenticular type. There are no obvious signs of recent major merger activity.
