The galaxy presents as a primarily smooth, elliptical object. It exhibits a yellowish-white hue concentrated in its central region, indicative of an older stellar population. There are no spiral arms or distinct disk structures visible. The galaxy appears slightly elongated, rather than perfectly spherical. Fainter blue emissions are present in the outer regions, which suggests some limited recent star formation within the galaxy. The overall morphology suggests this galaxy is likely a massive elliptical galaxy at a significant distance from our own. The presence of a small degree of blue light around the edges seems to indicate it is still slowly evolving.