The galaxy presents as a somewhat elongated, disk-shaped object, oriented approximately along a northeast-southwest axis. It exhibits a prominent central bulge, appearing brighter and more concentrated than the surrounding disk. The disk itself demonstrates a relatively smooth texture, with a gradual decrease in luminosity from the central bulge outward. There is a slight hint of dust lanes or spiral arm structures in the disk, but they are not sharply defined. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing merger activity and does not show any major disturbance. There is a smooth transition between the disk and the surrounding background, with a Sersic index suggesting a light profile shape that is consistent with the observation of a well-defined bulge with a diffuse disk.
