This galaxy exhibits a smooth, elliptical morphology. The light profile appears centrally concentrated, displaying a gradual decrease in intensity from the core outwards. There is a noticeable color gradient, with the central region exhibiting a yellowish-white hue, suggesting an older stellar population. The outer regions display a slightly redder tint, indicative of potentially dustier areas or a change in the stellar population. There is no apparent sign of spiral arm structure, disk component, or ongoing major mergers. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions with neighboring galaxies. Its overall rounded shape and lack of distinct features suggest it is a fairly evolved system, likely an elliptical galaxy with little current star formation.
