The galaxy presents a distinct spiral morphology. Its overall color profile indicates a notable presence of older stellar populations concentrated within a prominent central bulge. The disk component exhibits spiral arms characterized by regions of ongoing star formation, discernible through their bluer color. These arms wind relatively tightly around the central bulge, displaying an organized and symmetrical structure with an apparent number of spiral arms between two and four. The galaxy appears relatively undisturbed with no signs of major interactions or mergers. The light distribution suggests a galaxy primarily comprised of a disk component, exhibiting a moderate bulge. The absence of significant dust lanes are observed within the visible spectrum. 
