The galaxy presents as a centrally concentrated, smooth object with a relatively elliptical morphology. There is a distinct radial color gradient, with the central region exhibiting a yellowish-white hue, suggestive of an older stellar population. The outer regions display a more complex color profile with the appearance of a redder population of stars. No significant spiral arm structure is visible, nor are there signs of substantial dust lanes or recent major merger events. The galaxy appears relatively undisturbed, with a smooth light distribution suggesting a well-mixed stellar population. The galaxy's appearance is indicative of an evolved system, likely with a substantial spheroidal component and a relatively quiescent star formation history. 
