The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. The overall color is slightly red-shifted suggesting an older stellar population. There is a subtle disk-like structure visible, though it is not sharply defined, and appears as a slight flattening along one axis. No distinct spiral arms or prominent dust lanes are observed. The galaxy is moderately compact, but appears to be surrounded by a faint halo or extended stellar envelope. The general lack of blue color or clumpy star-forming regions indicates a low current star formation rate. No signs of major disturbances or ongoing mergers are readily apparent. The object is quite symmetrical.
