The galaxy presents as a spiral type. It exhibits a disk structure that is nearly face-on, with a discernible spiral arm pattern. The arms appear somewhat flocculent and are relatively tightly wound. There are at least two prominent spiral arms that can be traced from the inner regions outward.

The central bulge region appears relatively small, and there is evidence of a bar-like structure extending through the center of the galaxy. This bar may be moderately defined.

Overall, the disk of the galaxy exhibits a mottled appearance, suggesting ongoing star formation within the arms. The spiral arms are bluer in color, indicative of younger stellar populations. The disk otherwise is yellowish in color. There appears to be a possibility of a minor disturbance event or a possible interaction with another galaxy, considering the slight asymmetries in the disk.
