The observed galaxy presents as an edge-on spiral with a notable central bulge. The disk appears elongated and relatively smooth. A degree of asymmetry or subtle warp may be present along the galactic plane. No obvious dust lanes or distinct spiral arm structures are discernible. The galaxy exhibits a gradual change in luminosity from the central bulge outwards, with a faint, diffuse halo extending beyond the main disk. Color gradients suggest a possible change in stellar populations from the center to the outer regions of the galaxy. There are no visible signs of interaction with other galaxies, such as tidal tails.
