The galaxy presents as a spiral galaxy, viewed at an oblique angle. It exhibits a prominent disk structure, which is the dominant feature of the galaxy.

A central bulge region is visible, appearing concentrated and moderately bright with a yellowish color, suggesting an older stellar population. From what can be observed, the bulge size seems relatively small compared to the overall disk size.

Spiral arms appear present, although the viewing angle makes a detailed assessment challenging. There seems to be a distinct arm structure; these arms are fairly tightly wound around the bulge.

There is no strong evidence of an obvious bar feature. Disk has some blotchiness of star forming regions along the spiral arms. Disk is bluer than the bulge suggesting younger stellar population.

There is no strong sign of major mergers or extreme tidal disturbances. The galaxy is mostly undisturbed in appearance.
