The object presents as a spiral galaxy, observed at a redshift indicating significant distance. The morphology suggests a grand design spiral structure. The galaxy's color profile shows a concentrated yellowish core indicative of an older stellar population dominating the central bulge. This contrasts with the bluer spiral arms that extend from the central region, suggesting ongoing star formation within these arms. These appear fairly tightly wound. Dust lanes are subtly visible within the spiral arms, contributing to the observed color variations and obscuring some of the light from the stars behind them. No significant tidal disturbances or signs of a major merger event are immediately apparent, suggesting a relatively undisturbed evolutionary history. The galaxy has a prominent bulge and spiral arms which are well-defined. The disk of the spiral is not observed edge on. The overall structure suggests moderate mass, with a significant but not dominant bulge component.