The galaxy appears to be an elliptical or possibly lenticular galaxy, exhibiting a smooth, spheroidal morphology. A central, bright bulge is observed, surrounded by a more diffuse halo of light. The light distribution suggests a relatively old stellar population, with a yellow-reddish color gradient towards the core of the galaxy. No distinct spiral arms or dust lanes are visible. The galaxy appears relatively isolated, with no immediately apparent signs of tidal disturbances or ongoing mergers.
