The galaxy presents as a lenticular or early-type spiral, exhibiting a centrally concentrated bulge. Its shape is approximately elliptical, with hints of a faint, diffuse disk extending outward. The galaxy’s color profile indicates an older stellar population in the core region, shifting towards younger stars or active star formation in the outer disk. Faint tidal features are present, with one possible minor merger or disturbance evident in the disk structure. Overall, the system appears relatively quiescent. 
