The galaxy presents as a relatively smooth, centralized light distribution, lacking distinct spiral arms or a prominent bar structure. It appears largely elliptical or spheroidal in shape, with a high degree of circularity. There's a discernible color gradient, transitioning from a yellowish-white core to a more diffuse, reddish-orange outer halo. The absence of distinct features suggests a relatively old stellar population and limited ongoing star formation activity. There is no visual evidence of any major ongoing merger events or significant tidal disturbances affecting the overall morphology of the galaxy.
