The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright yellowish hue, suggestive of an older stellar population dominating the core. Moving outward from the core, there's a subtle transition to a bluer, less concentrated halo. Faint spiral arm structures may exist, but it's difficult to discern due to the resolution. The overall form appears largely undisturbed, displaying no obvious signs of major mergers or significant tidal interactions, with the possibility of minor disturbances. The round morphology indicates a system that is generally relaxed and well-formed.
