The galaxy appears as a centrally concentrated, relatively smooth, elliptical system. It exhibits a high degree of circularity in its overall shape. There is no discernible disk structure, spiral arm features, or bar. The light profile seems to decline smoothly from the center outward, suggesting a fairly uniform stellar population and dust distribution. There are no signs of major ongoing mergers or tidal disturbances, though a very subtle asymmetry in the outer regions cannot be ruled out. The dominant color is a muted yellow-white, indicative of an older stellar population and suggesting a relatively low rate of current star formation. The overall appearance is consistent with that of a mature elliptical galaxy at intermediate redshift.
