The galaxy presents a primarily smooth morphology, with a suggestion of subtle internal structure. Its shape is somewhat elongated, deviating from a perfectly circular form and tending more towards an intermediate roundedness. The color gradient indicates a concentration of older stellar populations in the central regions, appearing yellowish-white, which transitions outwards to a bluer hue in the less-defined periphery. The galaxy displays no obvious signs of major ongoing mergers or significant tidal disturbances, although there's a faint hint of possible minor asymmetry in the outer regions, potentially indicative of a past interaction or minor disturbance. Overall, the light distribution appears relatively even, suggesting a fairly evolved system with moderate ongoing star formation concentrated mostly in the outer regions.
