The galaxy presents as an edge-on spiral, or possibly a lenticular galaxy, exhibiting a flattened disk structure. A prominent central bulge dominates the galaxy's core, displaying a smoother texture and a yellowish-orange hue, which suggests an older stellar population. Dust lanes appear to be present, obscuring portions of the disk. A bluer region, perhaps indicative of younger stars or active star formation, is visible. Overall, the galaxy appears well-formed and relatively undisturbed, with no obvious signs of major recent mergers, though some minor disturbances cannot be ruled out. 
