The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. There's no clear evidence of spiral arms or a distinct disk component. The light distribution appears relatively uniform, fading gradually from the bright core. The color gradient suggests an aging stellar population, with a yellow-red hue dominating the galaxy's overall appearance. There's no visual indication of active star formation regions or significant dust lanes. There seems to be little to no disturbance of the primary galaxy shape, showing no signs of an on-going merger.
