The observed galaxy presents as a spiral type, exhibiting a well-defined disk structure. The orientation is approximately face-on, allowing for detailed examination of its spiral morphology. Two distinct spiral arms are present, demonstrating a moderate winding. These arms appear to emanate from a prominent central bar structure. The central bulge is small to moderate in size relative to the overall galactic disk, and the galaxy appears to be relatively undisturbed. The color suggests ongoing star formation, particularly within the spiral arms. The overall structure is consistent with a spiral galaxy at an intermediate redshift.
