The galaxy presents as a moderately elliptical structure. A bright, concentrated nucleus dominates the central region. The color gradient shifts from a warmer yellow-white core to a cooler blue-white in the outer regions, suggestive of differing stellar populations and possible ongoing star formation. The shape is close to round, with only a slight elongation. The galaxy appears undisturbed, without any major tidal features or signs of a recent merger. The outer edges of the galaxy fade smoothly into the background, indicating a gradual decrease in stellar density.
