This galaxy appears to be an elliptical galaxy at a moderate redshift. The light profile is smooth and centrally concentrated, lacking any distinct spiral arms or prominent features usually associated with disk galaxies. The color gradient suggests an older stellar population, possibly with ongoing low-level star formation, but not particularly active. There may be some evidence of minor tidal disturbance, but the overall morphology is undisturbed. The galaxy appears nearly circular in shape. Its apparent magnitude indicates a considerable distance, consistent with the measured redshift. The luminosity is relatively high for the apparent size, indicative of a massive galaxy.
