The galaxy presents a largely smooth, elliptical morphology, appearing mostly round. Its core exhibits a concentrated, bright, yellowish-white luminosity. The outer regions display a more diffuse, greenish-blue halo, suggesting the presence of some star formation activity, although modest. There is no evidence of prominent spiral arms or a distinct disk structure. The overall structure appears relatively undisturbed, lacking obvious signs of major mergers or significant tidal interactions. A slight asymmetry can be observed, but no prominent tidal tails or distortions are visible, suggesting a relatively relaxed, evolved system.
