The galaxy presents as an elliptical-like structure. It exhibits a generally smooth morphology with a noticeable central bulge. The light is relatively concentrated. There is a small portion of the galaxy that is not quite as smooth. A slight deviation in the main body of the galaxy hints at a possible interaction. The color gradients suggest that the core of this galaxy is composed of older stars and possibly dust, with a less prominent disk component exhibiting bluer, younger stellar populations. There is little sign of active star formation activity. The overall shape is mildly elongated but generally elliptical.
