The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a yellowish-orange hue, suggesting a stellar population that is relatively evolved, with a comparatively low rate of star formation. The galaxy presents an approximately rounded morphology. There are no obvious spiral arms or a prominent disk structure visible; its light is distributed in a spheroidal fashion. The galaxy may be undergoing or have undergone a recent merging event, as there seems to be disturbances in its general shape. Overall, the galaxy appears to be a fairly massive elliptical galaxy at intermediate redshift.
