The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is generally elliptical, exhibiting a high degree of circularity. The light profile appears to decline gradually from the center outwards with no obvious signs of spiral arm structures or a prominent disk. There is a slight color gradient observed within the galaxy; the central region is somewhat yellow, whereas the outer regions appear to be slightly redder. There are no readily apparent signs of significant tidal disturbances, strong asymmetry, or a major ongoing merger. Based on the observed characteristics, it is likely a high mass system with very low star formation. There is a small, faint point-like object in the center, which is likely an active galactic nuclei. The object is relatively compact with a consistent surface brightness.
