The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration, with a bright, relatively small core that diffuses outwards. The color appears to be slightly greenish/yellowish, possibly indicating an older stellar population, although some bluer elements cannot be ruled out. There is a subtle suggestion of a disk-like structure within the central regions, but this is not well defined. Subtle disturbances are present that indicate a past or ongoing interaction with a smaller galaxy. 
