The galaxy appears to be an elliptical galaxy. It exhibits a largely smooth, concentrated morphology. The light profile appears largely featureless with a high degree of central concentration. The galaxy exhibits a relatively round shape with a slight elongation. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The central region is very bright, with a color gradient, shifting from a pale yellow-orange at the core to a slightly bluer hue in the outer regions. This color gradient suggests that there are older stars in the center and younger stars more dispersed throughout the galaxy. There is a slight hint of a disk, but it may simply be the slight elongation of the galaxy.
