The galaxy presents an elliptical morphology, with a dominant smooth, centrally concentrated bulge. The overall color profile suggests a relatively evolved stellar population, with a yellowish-orange hue characteristic of older stars. While the image lacks fine detail, there is a slight elongation visible, deviating somewhat from a perfectly spherical shape. No distinct spiral arm structures are discernible, reinforcing the classification as an elliptical galaxy. There is no clear evidence of ongoing major mergers or significant tidal disturbances, the galaxy appears relatively undisturbed. 
