The galaxy presents as a spiral galaxy, potentially viewed at an oblique angle. It exhibits a prominent central bulge, surrounded by a relatively flattened disk structure. The disk features spiral arms, although they are not sharply defined and have a somewhat flocculent or patchy appearance. There is a slight asymmetry in the distribution of light within the disk, suggesting a possible mild disturbance or interaction. The galaxy exhibits a bluer color, indicative of ongoing star formation. A moderate amount of dust extinction and reddening is apparent, particularly within the spiral arms.
