The galaxy exhibits a spiral structure with distinct, well-defined arms. The spiral arms appear flocculent, showcasing active regions of star formation. These star-forming regions are bright and blue, indicating the presence of young, hot stars. There is evidence of dust lanes within the spiral arms, appearing as dark, obscuring bands. A central bulge is present, but it does not dominate the overall structure. The color suggests an older stellar population in this region, but it is not strongly pronounced, indicating that the galaxy is actively forming stars overall. The galaxy's disk is viewed at an intermediate inclination. There is no apparent strong central bar structure. There appears to be an interacting galaxy or a merging event occurring, as there is a noticeable disturbance or asymmetry in the outer regions of the spiral arms. The overall color suggests ongoing moderate levels of star formation activity.
