This galaxy presents a complex morphology, exhibiting characteristics of both a smooth elliptical galaxy and a disrupted system undergoing interaction. The galaxy's core appears relatively smooth and centrally concentrated, with a faint, diffuse halo extending outwards. However, superimposed on this smooth component are signs of tidal disturbances, including faint plumes or streamers of stellar material extending away from the main body. These tidal features suggest a possible recent or ongoing merger event with a smaller companion galaxy. The overall color of the galaxy is relatively red, indicating an older stellar population with fewer young, hot stars. There are indications of possible dust lanes or patches within the galaxy, which may be associated with the merging event or internal processes.
