The galaxy presents a somewhat elliptical morphology with a noticeable bulge. A slight disk-like structure appears to be present. The central region is dominated by a bright, concentrated core. Fainter extensions stretch outwards from this central area, but they are not well-defined. There appears to be some asymmetry in the outer regions of the galaxy. The overall color suggests a composition of older stellar populations, with a possible presence of ongoing, but low levels of, star formation. The galaxy displays a hint of a dusty spiral structure upon closer examination.
