The object appears as a relatively smooth elliptical galaxy, showing a concentrated central bulge. The core region exhibits a yellowish-orange hue, possibly indicating an older stellar population. This is surrounded by a fainter, more diffuse halo. The isophotes are generally elliptical, though there is a slight suggestion of a disk-like structure. No distinct spiral arms or dust lanes are apparent. The overall color suggests intermediate redshift, consistent with a sizable stellar mass. There is no obvious evidence of a major merger event.
