The galaxy presents as a spiral galaxy with a prominent central bulge. The bulge appears yellowish, suggesting an older stellar population. Faint spiral arms extend outward from the bulge, though their structure is not well-defined. The arms exhibit a bluish tint, indicating the presence of younger, hotter stars and ongoing star formation. The spiral arms appear tightly wound around the galactic center. The galaxy is not perfectly symmetrical, exhibiting a slight distortion in its overall shape. There is a suggestion of a possible bar structure in the central region, but it is not distinct. No signs of major mergers are apparent in the image, though subtle disturbances cannot be ruled out. Overall, it shows typical features of a late-type spiral galaxy.
