The galaxy presents as a relatively smooth, centralized structure. It exhibits a significant central bulge that dominates its overall morphology. The color gradient suggests an aging stellar population within the core. The lack of defined spiral arms or significant dust lanes points towards a later-type morphology, possibly an elliptical or lenticular galaxy. There is a suggestion of a slight disk structure. The overall color is reddish, indicating a lower rate of star formation. There is no apparent major merger activity or significant tidal disturbances.