The galaxy presents as a flattened, disk-shaped system, viewed at a significant inclination. It exhibits a bright, concentrated central bulge, appearing a yellowish-white hue indicative of an older stellar population. The disk shows a slightly bluer color than the bulge. Although somewhat indistinct, the galaxy gives a subtle suggestion of spiral arm structure within its disk. There is no immediately obvious evidence of any major ongoing merger activity or strong tidal disturbances.
