The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light profile increases towards the center, which appears bright and somewhat yellowish. The outer regions show a more diffuse distribution of light, with hints of a disk-like structure although the galaxy does not possess strong spiral arms. Some regions of blue light are detectable in the outskirts. The overall shape is largely elliptical but not perfectly so. There may be a slight asymmetry in the shape, possibly indicative of a minor interaction or disturbance. Evidence for ongoing or recent major mergers is not readily apparent.
