The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. Fainter, diffuse extensions surround the core, hinting at a disk-like structure. The disk appears relatively smooth. The galaxy exhibits a slight elongation in its overall shape. No distinct spiral arms are apparent. There is no visible evidence of any major ongoing mergers or significant tidal disturbances. The overall color profile suggests moderate star formation activity.
