The galaxy presents a generally smooth morphology, appearing elliptical in shape. The light distribution is concentrated towards the center, with a diffuse halo extending outwards. There is a lack of readily discernible spiral arms or significant substructure within the galaxy. The color appears yellowish-orange, possibly indicating an older stellar population. The galaxy does not display any obvious signs of tidal disruption or ongoing major merger events. Minor disturbances may be present. The overall appearance suggests a relatively evolved system.
