The galaxy presents as a centrally concentrated object with a generally smooth appearance. It exhibits an elliptical morphology, elongated slightly along one axis. A bright, compact core dominates the central region, suggesting a high concentration of stars. The color profile indicates a redder hue in the core, transitioning to a slightly bluer color in the outer regions, which may indicate the presence of younger stellar populations there. There is no evidence of strong spiral arm structure or distinct morphological features, such as a bar or prominent dust lanes. Subtle irregularities in the outer halo may suggest minor tidal interactions, though the galaxy appears largely undisturbed.
