The galaxy presents as a smooth, elliptical morphology with a dominant central bulge. It exhibits a yellow-orange hue, indicating an older stellar population. The galaxy appears relatively undisturbed, lacking any obvious signs of ongoing mergers or tidal interactions. The concentration of light suggests a high degree of central mass concentration. There is a slight elongation in its overall shape, deviating from a perfect circular form. Star formation appears to be minimal based on the color profile and lack of blue light.