The object appears to be a spiral galaxy at moderate redshift. Its morphology is dominated by a prominent disk structure. The spiral arms are well-defined, exhibiting a tightly wound pattern. Two distinct spiral arms are visible, emerging from a central bulge. The bulge itself appears moderately sized in relation to the disk. There is no obvious bar structure present. The galaxy appears relatively undisturbed, with no strong evidence of major merging activity, although subtle distortions could suggest minor interactions. Star formation appears present within the arms. The general color profile suggests a population of relatively young stars. The disk is not viewed edge-on.
