The galaxy presents as a centrally concentrated, smooth object. It exhibits a generally elliptical morphology, appearing mostly round in shape. The color profile shifts from a yellowish-white center to a greener edge. There are no obvious spiral arm structures or prominent dust lanes visible. The overall appearance suggests an evolved stellar population, with potentially older stars dominating the light output. No clear signs of major mergers or significant tidal disturbances are observed, though a possible minor asymmetry could warrant further investigation with higher-resolution data. 
