This galaxy exhibits a clear spiral structure, with well-defined arms emanating from a central region. The spiral arms are populated with regions of active star formation, indicated by their bluish color. Patches of redder hues are also observed within the arms, possibly indicative of older stellar populations. The central bulge appears relatively small. There is no obvious evidence of a strong central bar. The overall morphology suggests an intermediate stage spiral galaxy. There is a subtle but noticeable asymmetry in the arm structure, potentially indicative of a past or ongoing interaction. There are no obvious signs of a major merger, although a minor interaction or disturbance cannot be ruled out.
