The galaxy presents as a fairly smooth, centrally concentrated object, with an elliptical morphology. It exhibits a roughly spherical shape. There are no clear signs of spiral arms or a prominent disk. Some minor irregularities are present, but the overall structure appears undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. The color profile indicates a dominant older stellar population, likely with relatively low levels of ongoing star formation. The galaxy shows a hint of a redder core, possibly indicating dust accumulation or a change in stellar populations toward the center. 
