The galaxy presents as a somewhat smooth, disk-like structure, though the smoothness is disrupted by hints of internal features. These features appear as a brighter central region surrounded by what may be spiral arms, however, these arms appear diffuse and ill-defined. The galaxy displays a color gradient, appearing bluer towards the outer edges and redder towards the center, potentially indicating differing stellar populations or dust obscuration. There may be minor disturbances suggesting a possible ongoing or recent interaction or merger event, based on the disturbed arm structure. The galaxy is relatively compact.
