The galaxy presents a clear disk structure. It is inclined substantially relative to our line of sight.  The overall shape appears elliptical due to this inclination.

The central region displays a bright, concentrated luminosity, indicative of a substantial bulge.  The bulge color appears more yellow/orange in comparison to the disk.

Spiral arm structures are apparent, although somewhat flocculent. The arm structure is not sharply defined.

The disk exhibits noticeable color variation, with bluer hues apparent in the outer regions, which suggests active star formation. Dark dust lanes may be present, silhouetted against the starlight of the disk. The light is more diffuse further out in the disk.
