This galaxy appears to be an elliptical galaxy at a considerable distance, indicated by its redshift. Its light profile suggests a generally smooth and centrally concentrated distribution of stars. The galaxy exhibits a roughly elliptical shape, appearing mostly round. The central region is bright and yellowish-orange, which could be indicative of an older stellar population dominated by evolved stars. The outer regions are fainter and exhibit a subtle gradient of color, potentially hinting at differences in stellar populations or dust content as one moves outwards from the core. There is little evidence of significant spiral arm structure or distinct features indicating ongoing major mergers or disturbances.
