The object appears to be a spiral galaxy, observed at a redshift indicating a substantial distance. The galaxy exhibits a moderately sized central bulge, with spiral arms that are fairly tightly wound. These spiral arms are prominent and show signs of active star formation. The galaxy exhibits colors indicative of a significant population of young, hot stars, and a more significant population of older, redder stars in the bulge. The disk appears relatively undisturbed, and there is no clear evidence of major ongoing mergers or strong tidal interactions with other galaxies, although it looks like there could be a minor disturbance. There is a possible weak bar structure observable across the central region. The galaxy does not appear to be observed edge-on. The overall morphology suggests an intermediate-mass spiral galaxy with ongoing star formation within its spiral arms.
