The galaxy presents as a generally smooth, elliptical-like object, with a concentrated central bulge that emits strongly. There is also some fainter, diffuse light surrounding the bulge. Its color appears to be predominantly orange, with a slight shift towards red. This suggests an older stellar population. The galaxy appears fairly round, with only a slight elongation. There is no obvious spiral structure present in the available imagery, and no signs of an ongoing major merger, although there may be some minor disturbances. Its overall high mass corresponds to the image of a large, smooth, and generally uniform galaxy, which has largely ceased its star formation.