The galaxy presents as a single, centrally concentrated object with a generally smooth morphology. Its overall shape appears somewhat elliptical, deviating slightly from a perfect circle. A bright, yellowish core dominates the central region, suggesting a higher concentration of older stars. Fainter, diffuse light extends outwards from the core. There is a hint of bluer light within the diffuse outer regions. The object seems largely undisturbed, without any signs of major ongoing merger activity or significant tidal distortions. A slight asymmetry is present, possibly indicative of a minor interaction or internal dynamics. The galaxy has an estimated size that is typical for galaxies of this type. Given its colors, mass, and undisturbed morphology, it is classified as a massive, relatively passive system with a low star formation rate.
