The object appears to be a spiral galaxy, observed at a redshift suggesting intermediate distance. It presents a noticeable disk structure, with a predominantly blue hue indicating active star formation. The spiral arms, though somewhat indistinct, imply a grand design morphology. A central bulge is visible, exhibiting a yellowish color, suggestive of an older stellar population. The galaxy is neither perfectly face-on nor edge-on, but rather at a slightly tilted orientation with respect to the observer. There is no evidence of any major merging activity, although some minor disturbances cannot be ruled out. Overall, the galaxy demonstrates characteristics typical of late-type spiral galaxies with ongoing star formation.
