The object is a spiral galaxy, exhibiting a distinct disk structure with prominent spiral arms. The arms are loosely wound, extending outwards from a central bulge region. The bulge appears relatively small compared to the overall size of the galaxy. The disk shows evidence of ongoing star formation, indicated by the bluish tint. The galaxy may be undergoing some form of disturbance or interaction. The morphology suggests a galaxy with a moderate amount of internal structure and a relatively low mass. There is no significant bar structure apparent in the central region.
