This galaxy exhibits a distinct spiral structure. The arms appear flocculent and somewhat tightly wound, wrapping around a prominent central bulge. The bulge displays a yellowish hue, likely indicating an older stellar population. The spiral arms show a bluer color, suggesting ongoing star formation. There is evidence of a central bar structure bisecting the bulge, possibly influencing the spiral arm morphology. Dust lanes are visible within the spiral arms, obscuring some of the light from behind. There is no apparent signs of tidal features or major mergers. The galaxy has a noticeable disk and appears to be viewed at an angle that is slightly less than edge on.
