The galaxy presents a distinct spiral morphology, although the arm structure appears somewhat flocculent. The winding of the spiral arms is moderately tight. A central bulge is evident, exhibiting a yellowish hue that suggests an older stellar population. The blue color of the spiral arms suggests that the galaxy is actively forming new stars. The lack of strong dust lanes is noteworthy. There is no sign of a major ongoing merger, however, some small disturbance cannot be ruled out.