The galaxy presents a distinctly barred spiral structure. The bar appears prominent and well-defined, oriented at an angle relative to our line of sight. Two tightly wound spiral arms emanate from the ends of the bar, exhibiting a moderate pitch angle. These arms show subtle variations in color and luminosity, suggesting differing stellar populations or star formation activity along their lengths.

The galaxy's central bulge is relatively small compared to the overall galactic disk. The disk itself displays a flattened morphology, and the galaxy appears to be a bit edge-on, meaning that it is tilted from our point of view. There is little evidence of strong disturbances or major mergers in this galaxy, though a minor disturbance cannot be completely ruled out.
