The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a high degree of roundness. The core exhibits a bright, yellowish hue, which gradually fades into a greenish-blue halo. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy shows no signs of major mergers or significant tidal disturbances in its immediate vicinity, and the surrounding regions appear relatively undisturbed. Overall, the galaxy appears to be an evolved system, potentially with a reduced rate of active star formation.
