The galaxy exhibits a flattened, disk-like morphology with a noticeable central bulge. The light distribution appears smooth, especially near the center. Faint hints of a spiral structure are suggested by subtle variations in color and brightness within the disk, though these arms are not well-defined. The overall shape appears undisturbed, lacking any obvious signs of ongoing major mergers or tidal interactions. There is a slight asymmetry in the light distribution. The galaxy possesses a bright, concentrated nucleus. Faint extended emission emanates perpendicular to the disk, possibly outflow from the nucleus.
