The galaxy presents a distinct spiral structure. Several spiral arms emanate from a moderately bright central bulge, exhibiting a multi-armed morphology. The arms appear to be relatively tightly wound near the core but then fan out. The disk component appears to be the dominant feature, with the spiral arms defined by concentrations of bluer regions, possibly indicating areas of active star formation. Patches of redder material appear throughout the arms. No obvious bar structure is readily apparent in the central region. The overall structure exhibits some degree of disturbance or asymmetry; the outer regions of the spiral arms are somewhat uneven, potentially indicative of minor gravitational interactions. The central bulge appears relatively smooth, although the limited resolution does not allow for detailed assessment.
