The galaxy presents a primarily face-on orientation relative to our line of sight, exhibiting a distinct spiral structure. The spiral arms are tightly wound, emanating from a central bulge that appears to be of moderate size. Dust lanes are visible within the disk, contributing to the galaxy's overall morphology. There is evidence suggesting a possible weak bar structure bisecting the central bulge region. The disk component is the dominant feature, outshining the bulge. There are two primary spiral arms that are distinct. The galaxy does not show any obvious signs of a major disturbance or merger event, and it appears to be relatively isolated in its environment.
