The galaxy presents as a relatively smooth, elliptical form with a notable central bulge. Its overall color appears yellowish-orange, suggesting an older stellar population dominates the light emission, though bluer regions are observed in the outer edges of the galaxy. There is a slight elongation, giving it an oval shape rather than perfectly circular. While the bulk of the galaxy appears undisturbed, subtle irregularities in the light distribution suggest the possibility of minor interactions or internal processes influencing its structure. The galaxy's mass suggests that this is a large, well-developed galaxy. The data suggests that the rate of new star formation is low.