The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology, though it appears close to round. A dominant central bulge is evident, exhibiting a yellowish-red hue suggestive of an older stellar population. Fainter, diffuse light extends outward from the core. There is some evidence of tidal disturbances or interaction with a smaller galaxy, with possible ongoing or recent minor merging activity. Overall, the system is consistent with an early-type galaxy, likely an elliptical. It appears to be relatively quiescent in terms of current star formation.
