The object appears to be a single, relatively smooth galaxy at a cosmological distance, as evidenced by its redshift. It exhibits a concentrated, roughly circular morphology, indicating a lack of significant spiral arm structure or a dominant disk. The galaxy presents a yellowish-orange hue, suggesting an older stellar population. There is an apparent absence of significant dust lanes or active star-forming regions within the galaxy as observed by its color and smoothness. There is little to no disruption in the surrounding field and it is unlikely that this galaxy is undergoing major mergers. Based on its features it is likely that this is an elliptical galaxy. 
