The galaxy presents a spiral morphology, viewed at an oblique angle. A prominent central bulge is evident, surrounded by a disk structure that displays discernible spiral arm features. The arms appear somewhat flocculent and extend outwards from the central region.

The overall color of the galaxy is bluish, particularly in the outer regions of the disk, suggestive of ongoing star formation. There are hints of dust lanes within the disk. A weak bar-like structure may be present within the central region. The galaxy exhibits a moderate level of internal structure. There are no apparent signs of major mergers or significant tidal disturbances.
