The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge that is more luminous and a more yellow to orange color. The halo gradually fades away. The overall shape is close to round and there is no prominent evidence of strong spiral arm structures or major disturbances. The galaxy appears largely isolated, with no obvious signs of ongoing merger activity or significant tidal interactions with nearby galaxies. The observed color suggests a relatively older stellar population and a low rate of star formation.
