The galaxy presents as a single, concentrated object with a smooth light distribution. It appears elliptical in shape, with a high degree of central concentration. The light profile indicates a dominant bulge component with a gradual decrease in surface brightness outwards. The primary color is yellowish-white, suggesting an older stellar population with fewer young, blue stars and relatively low ongoing star formation. There is no evidence of spiral arms, dust lanes, or other distinct morphological features. The galaxy appears undisturbed, without any signs of tidal interactions or recent mergers.
