The galaxy presents a somewhat face-on orientation relative to our line of sight, displaying a distinct spiral structure. The spiral arms appear relatively tightly wound, originating from a central bulge region that occupies a significant portion of the galaxy's diameter. This bulge exhibits a moderate size, with a smooth, diffuse appearance. A faint bar-like structure seems to bisect the central region. 

The spiral arms themselves are not particularly well-defined, showing more of a flocculent or patchy texture rather than long, continuous features. They exhibit a bluer color indicative of ongoing star formation activity. There are no signs of significant tidal disturbances or interactions with other galaxies.
