The galaxy presents as a centralized, somewhat elliptical object. It has a bright, condensed core region, surrounded by a more diffuse halo of light. The light from the central bulge appears primarily white or slightly bluish-white, which could indicate a population of hotter, younger stars or ongoing star formation in the nuclear region. The outer regions of the galaxy exhibit a fainter, smoother texture with hints of a disk shape. There are subtle indications of minor disturbances or asymmetries within the galaxy's structure, possibly indicative of interactions with other galaxies, or recent accretion events. There is little dust visible within the galaxy.