The galaxy exhibits a clear spiral structure, viewed at a significantly tilted angle relative to our line of sight. The disk of the galaxy appears thin and elongated due to this inclination.

Two prominent spiral arms are visible, extending outwards from the central bulge. These arms display a medium winding, neither tightly wound nor loosely defined. There's a hint of patchiness within the spiral arms, which suggests the presence of star-forming regions.

The central bulge is noticeable but not overwhelmingly dominant, appearing relatively small in comparison to the overall size of the disk. Its color is generally yellower than the arms, indicating an older stellar population. A strong bar-like structure is evident across the central region of the galaxy, bisecting the bulge. The galaxy may be undergoing a minor disturbance due to interactions with surrounding objects.
