The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a reddish-brown periphery, which could suggest variations in stellar population. There are no apparent signs of spiral arm structures or significant dust lanes. The overall morphology suggests an evolved system with suppressed star formation, potentially a lenticular or early-type spiral galaxy nearing the end of its star forming lifecycle.
