The galaxy presents as a largely featureless elliptical or S0-type system. A concentrated central bulge dominates the light profile, with a smooth, relatively symmetrical halo extending outwards. The core region exhibits a yellowish-orange hue, indicative of an older stellar population, while the outer regions appear slightly bluer, hinting at some more recent, though subdued, star formation. There is no apparent spiral structure, dust lanes, or significant tidal distortions. The overall appearance suggests a dynamically relaxed system. There is a very slight hint of a disk.
