The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, compact profile, transitioning to a slightly bluer, more diffuse halo. There is little evidence of significant spiral arm structure or well-defined dust lanes. The colour profile suggests a moderate amount of on-going or recent star formation. The outer regions are less well-defined and show hints of tidal disturbances or interactions, but overall the galaxy appears largely undisturbed.
