The galaxy presents as a concentrated, centrally luminous object. Its morphology appears largely smooth, with a high degree of radial symmetry in its light distribution. There is no apparent structure such as spiral arms or a distinct disk. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish-white core to a redder halo, indicating a possible differential in stellar population or dust distribution. Given its general spheroidal shape and color profile, the galaxy is likely an elliptical galaxy. It is moderately bright, suggesting a considerable integrated stellar mass, yet its star formation activity is presumably very low. There is no visual evidence suggesting ongoing or recent major mergers or interactions. Minor disturbances cannot be ruled out but are not readily visible. The galaxy has a intermediate roundness.
