The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge of high luminosity dominates the structure, exhibiting a yellowish-white hue indicative of an older stellar population. The luminosity appears to gradually decrease from the center outwards. The outer regions display a fainter, more diffuse halo with subtle hints of a disk-like structure that is nearly edge on. There may be a few faint and unresolved features, possibly indicating minor disturbances within the galaxy. The overall impression is that of a relatively isolated, evolved system.
