The galaxy presents a generally smooth morphology, appearing largely featureless. The light distribution suggests a centrally concentrated spheroid, exhibiting an elliptical or lenticular galaxy type. The core is bright and yellowish, potentially indicating an older stellar population dominating the central region, possibly with a supermassive black hole at the center. Fainter, bluer regions are very slightly observable around the center. No distinct spiral arm structures or significant dust lanes are apparent. There's a subtle color gradient, with the central bulge appearing more yellow and red, and the outer regions appear slightly bluer. This suggests a possible difference in stellar population ages or metallicities. There is no significant evidence of any major ongoing merging activity or significant tidal disturbance. There is very little visual appearance of star formation, so it is likely quiescent.
