The observed galaxy presents as a spiral type. It exhibits a notable disk structure with discernible spiral arms. These arms appear to be somewhat tightly wound around a moderately sized central bulge.

There is a strong suggestion of a bar-like structure spanning across the central region of the galaxy, adding to the complexity of its morphology. The disk is oriented approximately face-on relative to our line of sight.

There are some indications of mild irregularities or disturbances within the disk, potentially suggesting minor interactions or internal processes. Overall, the galaxy appears to be relatively isolated, without obvious signs of a major merger event. The blue hue suggests ongoing star formation.
