The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears uniform throughout the galaxy, with a gradual fading towards the outer edges. Color gradients suggest that the core of the galaxy is composed of older stellar populations, whereas the outer regions appear bluer, which could point to pockets of young stars. There might be a faint disk structure. There is a second dimmer blue area above the galaxy, so the galaxy is likely undergoing a minor merger. There are no signs of significant tidal disturbances or prominent dust lanes.
