The galaxy presents as a centrally concentrated elliptical system. The core exhibits a high surface brightness with a smooth, even luminosity profile that gradually decreases outwards. Color gradients suggest a stellar population that is generally old and passively evolving.

The galaxy appears largely undisturbed, lacking any significant tidal features or evidence of recent major mergers. There is no apparent spiral structure. The galaxy displays a roughly round morphology with a slight ellipticity. The absence of distinct features points towards a galaxy that has largely exhausted its gas supply and is no longer actively forming stars at a significant rate.
