The galaxy appears to be an edge-on spiral, characterized by a flattened, disk-like structure. The central bulge is not particularly prominent, suggesting it may be a smaller fraction of the total galactic mass. A dust lane is observed, bisecting the galaxy along its major axis, indicating the presence of significant interstellar dust within the galactic plane. The bluer color suggests recent or ongoing star formation. The galaxy appears relatively undisturbed, without obvious signs of major mergers or tidal interactions.