The observed galaxy presents a spiral morphology, exhibiting a prominent disk structure. Within the disk, spiral arms are clearly discernible, with a predominantly wound structure. The galaxy appears to possess a noticeable bulge component, estimated to be a moderate size relative to the overall structure. Dust lanes are visible throughout the galaxy, particularly along the spiral arms. The central region of the galaxy exhibits a bright, concentrated luminosity, possibly indicating the presence of an active galactic nucleus or a region of enhanced star formation. There appears to be no dominant bar structure in this galaxy. There are no signs of major disturbances to the galaxy, suggesting that it is not undergoing a major merger.