This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and spheroidal morphology. There is a highly concentrated central bulge, potentially indicating the presence of a supermassive black hole. The light profile diminishes gradually from the center outwards, and its overall shape is approximately in between round and elliptical, with no distinct spiral arm structures or prominent features like dust lanes or star-forming regions visible in this image. The core region presents a yellowish hue, possibly caused by an older stellar population. This galaxy shows no apparent signs of major interaction or tidal disturbances that would suggest a recent merger event. It does, however, exhibit slight asymmetry, potentially indicating minor gravitational interactions.
