The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, with a gradual decrease in surface brightness towards its outer regions. The galaxy appears almost spheroidal in shape. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's color index suggests a population of older stars with modest levels of star formation. There is no obvious indication of ongoing merger activity or tidal disturbances. The galaxy seems to be relatively isolated in its environment.
