This galaxy appears to be a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy at intermediate redshift. The color suggests a population of older stars, as indicated by its redder appearance in the r and z bands compared to the g band, and a low current star formation rate. The galaxy exhibits a roughly round shape and is fairly compact, with an effective radius indicating it is a typical galaxy size. There is no apparent major disturbance in its morphology, suggesting it is not currently undergoing a significant merger event, and is not an artifact.
