The galaxy presents as a disk-shaped system, seen at an oblique angle. The central region exhibits a bright, concentrated bulge, appearing smooth and yellowish-white. The disk shows a mottled texture, with hints of spiral arm structure. The disk component displays a blueish hue in regions surrounding the central bulge, with a darker periphery. The overall form is relatively undisturbed, showing no obvious signs of major merger activity or strong tidal distortions. The light distribution appears centrally concentrated, with a smooth transition from the bulge to the disk. The galaxy seems to be dominated by older stellar populations in the central regions, with ongoing star formation in the surrounding disk.
