The object is a spiral galaxy, observed at a redshift indicating a moderate cosmological distance. The galaxy exhibits a well-defined disk structure with prominent spiral arms. The morphology suggests a classification as a barred spiral, though the bar feature is not highly pronounced. 

The central bulge is moderately sized, contributing significantly to the overall luminosity. The spiral arms are wound moderately tightly, with a pitch angle that suggests ongoing star formation. The arms appear relatively symmetrical and extend outwards from the bar/nuclear region. 

Color gradients across the galaxy indicate varying stellar populations, with bluer regions correlating with active star formation in the spiral arms. The disk is viewed at a nearly face-on orientation, minimizing obscuration. The galaxy does not present any visible signs of major interaction or recent merger events, appearing relatively undisturbed in its morphology.
