The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated brightness profile, with a gradual decrease in luminosity towards its outer regions. The color appears generally yellowish, possibly indicating a population of older stars. There is a very slight indication of bluer components. There is no pronounced disk structure or spiral arms readily apparent. There is no clear indication of ongoing major merger activity or significant tidal disturbances. The galaxy presents as a fairly isolated system with a regular, spheroidal morphology.
