The galaxy presents a morphology consistent with a spiral galaxy, observed at a moderate inclination. Evidence of spiral arm structure is present, exhibiting a somewhat diffuse nature. The central bulge region shows a moderate size relative to the overall galactic disk. There appears to be a weak bar-like structure transecting the central bulge, although this feature is not strongly defined. The galactic disk displays a non-uniform color distribution, showing potential for recent star formation. There is no overwhelming evidence to suggest the galaxy is undergoing a major merger event, though a minor disturbance cannot be fully excluded. The disk component appears significantly more prominent than the bulge. Overall, the morphology suggests a galaxy with ongoing stellar formation and a somewhat perturbed disk structure.
