The object presents as an elongated, disk-shaped galaxy viewed nearly edge-on. A central bulge region is discernible, exhibiting a relatively smooth and concentrated light distribution. The disk component shows an extension in the vertical direction relative to its rotational axis. Hints of possible asymmetries within the galactic disk might suggest a minor gravitational interaction. The overall color distribution appears relatively uniform, lacking distinct features or prominent dust lanes along the mid-plane. The galaxy exhibits an elongated morphology which is characteristic of a spiral galaxy viewed edge-on. It displays a smooth profile, with a more concentrated central bulge.
