The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears to be a yellowish-white, suggesting an older stellar population. The galaxy exhibits a concentrated central bulge that is brighter than the outer regions. There is very little, if any, evidence of spiral arms or significant dust lanes. It appears to be an isolated galaxy without any signs of major interaction or merging events. The light profile decreases gradually from the center outwards, with no distinct features beyond the smooth, diffuse halo. The rounded shape and lack of prominent disk features support the classification of this galaxy as likely elliptical, possibly exhibiting properties of an S0-type galaxy.
