The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting an elliptical morphology. There is a general lack of defined spiral arms or a prominent disk structure. The light profile appears to be largely spheroidal in nature, decreasing gradually from a bright core outward.

Color gradients within the galaxy are subtle. The central region presents a slightly bluer hue, suggesting the presence of a younger stellar population or ongoing star formation in the core. The outer regions appear comparatively redder, possibly indicating an older stellar population. 

There is no readily apparent evidence of any major ongoing merger activity or significant tidal disturbances, with a generally undisturbed, relaxed appearance. The overall form indicates a galaxy that has likely undergone significant evolution and settling.
