The galaxy presents a largely smooth, elliptical morphology. A bright, relatively uniform central bulge dominates the structure. There is minimal evidence of spiral arm structure or distinct features. A slight elongation is observed, deviating from a perfectly circular form. The color gradient suggests a stellar population primarily composed of older stars, with a potential hint of ongoing, but subdued, star formation activity indicated by a slight bluish tinge. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
