The galaxy presents as a relatively compact, smooth object, appearing primarily bluish-white in color. The morphology suggests an elliptical or lenticular classification. The light distribution is concentrated towards the center and falls off gradually outwards, with no discernible spiral arm structure. The overall shape is somewhere between perfectly round and elongated. There is little evidence of ongoing major merging activity or significant disturbances, suggesting this galaxy may be relatively settled. The color indices indicate a moderate population of younger, bluer stars.
