The galaxy presents as an elliptical or lenticular type, appearing largely smooth and spheroid. It exhibits a concentrated central bulge that transitions smoothly into a more diffuse halo. There are hints of a very faint disk, but no strong spiral arms or bar structure is evident. 

Color gradients suggest an older stellar population, indicated by the yellow-orange hue dominating the galaxy's core. The outer regions show bluer tinges, suggestive of some, albeit limited, ongoing star formation.

There are some possible faint tidal disturbances or minor asymmetrical features but they are not clear. The bulk of the galaxy appears relaxed and well-formed. No clear signs of on-going mergers are visible, however the hint of disturbances around the galaxy could suggest a recent interaction. 