The galaxy presents as a centrally concentrated, elliptical-like structure. A bright, relatively compact core region transitions into a more diffuse, extended halo. The color profile suggests a dominant population of older stars, particularly in the central region, indicated by the reddish-yellow hue. Fainter, bluer light appears in the outer regions, hinting at the presence of younger stars or a modest amount of on-going star formation, though at a low rate. There is no discernible spiral structure or prominent dust lanes. The galaxy appears largely undisturbed, with no major signs of tidal interactions or recent mergers. Its morphology is generally smooth with a slight elongation; it is more in-between round and cigar-shaped. Faint disturbances are possible within the galaxy.
