The galaxy presents as a largely elliptical morphology, though potentially exhibiting a flattened disk-like structure when viewed from this angle. The central bulge is prominent and exhibits a concentrated, bright yellowish-white luminosity, likely indicating an older stellar population. The overall color gradient shifts towards slightly redder hues in the outer regions, with the most distant areas appearing relatively diffuse. There is no clear evidence of spiral arm structures or significant dust lanes, and the galaxy appears relatively undisturbed.
