The galaxy appears as a singular, fairly symmetrical, elliptical-like structure. It displays a relatively smooth light distribution, showing a high degree of central concentration and a slight elongation, not quite spherical. The color is a warm hue, trending towards redder wavelengths, suggesting an older stellar population dominates the light output. Evidences point to the possibility of it being a massive galaxy, with limited ongoing star formation. There are no apparent signs of recent mergers or major disturbances in its morphology, though a small percentage of disturbances cannot be ruled out. 
