The galaxy presents as a moderately bright, flattened system with a notable central bulge. The overall structure appears disk-like, possibly seen close to edge-on. The central region exhibits a high concentration of light, suggesting a prominent nucleus. Proceeding outwards from the center, the light distribution diminishes smoothly into a more diffuse, extended halo or disk. The color distribution shows a general trend of bluer hues in the outer regions, potentially indicating younger stellar populations or ongoing star formation, while the central bulge appears redder, suggestive of older stars. There may be a faint dust lane or asymmetry along the major axis.
