The object appears to be a spiral galaxy at a significant redshift. The galaxy exhibits prominent spiral arms, wound somewhat tightly around a central bulge. The bulge appears relatively moderate in size compared to the overall galactic disk. The disk shows a range of stellar populations, with a notable color gradient from the inner regions to the outer arms. The color indicates active star formation within the spiral arms and older stellar populations within the central bulge. There are no obvious signs of a significant bar structure. The galaxy appears relatively undisturbed with no major signs of an ongoing merger with another galaxy or other disturbances. The spiral arms are the dominant feature, indicating that the galaxy has a disk-like structure. The galaxy appears to have two distinct spiral arms. The image shows a possible slight disturbance, but is mainly showing its features.
