This galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. The outer regions gradually fade into the background sky, showing a diffuse halo. There is little evidence of spiral arms or prominent dust lanes. The overall color suggests a population of older stars. While the galaxy appears mostly uniform, subtle color variations are present. There is a slight redness to the core with bluer hues dominating in the outer regions. Based on the light profile, the object is well-defined. There is no obvious signs of tidal disturbances, nor the presence of ongoing major mergers.
