The galaxy appears to be a relatively smooth, elliptical-type galaxy at a distance indicated by its redshift. It exhibits a concentrated central bulge that gradually fades towards its outer edges. Its overall shape is quite round, with only a slight deviation from perfect circularity. There is a hint of a surrounding halo or envelope, though it is faint. No prominent dust lanes or spiral arm structures are discernible. The galaxy's color suggests an older stellar population with a relatively low rate of on-going star formation. There may be some minor disturbances in its form, suggesting it is a result of previous galaxy mergers or interactions.
