The galaxy exhibits a distinct spiral morphology, with a notable disk structure. The spiral arms appear tightly wound. A bulge is clearly visible, though it appears relatively small compared to the overall disk size. The central region displays a brighter, more concentrated luminosity, suggestive of a higher stellar density. Patches of blue-ish color are distributed throughout the spiral arms, possibly indicating regions of active star formation. There seems to be a bar-like structure and/or a slight asymmetry in the galaxy's structure, hinting at a potential interaction or internal dynamic process. There is evidence that some of its light has been redshifted.
