The galaxy appears as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge with a gradual fading towards the outer edges. The light distribution suggests minimal substructure, with a dominant smooth component. The color profile indicates a redder hue, implying an older stellar population. There's no apparent dust lane or spiral arm structure visible within the resolution of the image, which suggests a lack of ongoing active star formation and a more evolved system. The morphology indicates a relaxed structure with no significant signs of recent mergers or major disturbances, though minor disturbances cannot be ruled out. The galaxy exhibits an approximate size of just over 6 kpc. 
