The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades towards the outer edges. There is little indication of spiral arms or other distinct features typically associated with disk galaxies. The overall color appears somewhat redder than that of younger, star-forming galaxies, which would point to a more evolved stellar population. There is no evidence of any ongoing merging activity or major tidal disturbances. Faint hints of blueish light are present in the outer edges of the galaxy. The galaxy seems to be mostly undisturbed and relatively isolated. 
