The galaxy appears to be a spiral, observed at a redshift indicating a considerable distance. It exhibits a bright, concentrated central bulge, surrounded by a relatively smooth, yet distinct disk. The disk does not present sharply defined spiral arms. Instead, the spiral structure manifests as diffuse, flocculent regions of star formation that are more prevalent on one side of the galaxy.

The central bulge appears yellowish-white, suggesting a population of older stars. Conversely, the disk regions show a bluer hue, indicative of ongoing star formation within. A faint, extended halo of diffuse light surrounds the main body of the galaxy. The overall shape of the galaxy is elongated, showing some degree of flattening. There is a subtle indication of possible tidal distortion or interaction on one side of the galaxy, implying a past or ongoing gravitational interaction. The light distribution suggests a galaxy dominated by a relatively old stellar population in the bulge, with ongoing but moderate star formation in the disk.
