This galaxy presents a largely smooth, elliptical morphology. The core exhibits a concentrated, bright luminosity profile, suggesting an older stellar population dominating the central region. A subtle color gradient is observed, with the central region appearing more yellow/orange, transitioning to a slightly bluer hue in the outer regions. This suggests that the central bulge is dominated by older stars while more star formation is occurring in the outer regions. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy appears relatively undisturbed, exhibiting no strong tidal features or indications of recent major merger activity. The overall roundness of the galaxy is apparent, with the ellipticity being minimal.
