The galaxy presents as a spiral structure with a prominent central bulge. The spiral arms are distinctly visible, demonstrating a winding pattern that transitions from tightly wound to more open as they extend outwards from the core. The arms appear somewhat flocculent, exhibiting a patchy distribution of star formation regions.

There is a suggestion of a bar-like structure traversing the central bulge. The disk of the galaxy is inclined with respect to our line of sight but not fully edge-on, allowing a clear view of the spiral pattern. The bulge itself appears relatively small in proportion to the overall size of the disk. The overall color of the galaxy is bluish, indicative of a population of young, hot stars. The galaxy does not exhibit any strong signs of a major ongoing merger event, though there might be minor disturbances in the disk.
