The galaxy presents a generally smooth and elliptical morphology, suggesting classification as an elliptical galaxy or potentially a lenticular galaxy viewed close to face-on. The central bulge is prominent and exhibits a yellowish hue, likely indicating an older stellar population. The outer regions display a bluer color, suggesting the presence of some younger stars or ongoing star formation, although the overall star formation rate appears relatively low. There is no clear evidence of spiral arms or a distinct disk structure. Some minor disturbances or faint tidal features are possibly present, indicating the potential for past or ongoing interaction with another galaxy, however a major merger is unlikely. The overall structure indicates a system dominated by random stellar motions and triaxial in shape. 
