The galaxy presents as a relatively compact and smooth object. It exhibits a centrally concentrated morphology, with a bright, roughly circular core. The radial color gradient suggests a possible evolution in stellar populations, with the central region appearing more yellow/orange than the outer regions, possibly indicating older stellar populations in the core. The outer regions display a faint, diffuse blue halo surrounding the core. There is no visible evidence of spiral arm structure or significant dust lanes. The overall structure suggests a lack of ongoing major merger activity, with a relatively undisturbed, relaxed morphology. The galaxy's estimated effective radius indicates a moderate size.
