The galaxy exhibits a prominent disk structure characterized by two well-defined spiral arms that dominate the morphology. The arms appear somewhat flocculent, suggesting active star formation regions distributed along their lengths. A central bulge is discernible, displaying a moderate size relative to the overall galactic disk. There is evidence of a bar-like structure bisecting the bulge, although it does not appear overly pronounced. The galaxy's winding pattern appears medium. There is a faint indication of disturbance in the disk potentially due to minor interactions or mergers. There are no clear indications of a merging event.
