The galaxy presents as a centrally concentrated elliptical morphology. It exhibits a smooth, largely featureless profile with a high degree of radial symmetry. A subtle color gradient is observed, with a slightly bluer hue in the outer regions transitioning to a more yellow-red color towards the galactic core. This may indicate a younger stellar population in the outer regions compared to the core. No significant tidal features, dust lanes, or other prominent morphological disturbances are apparent. The overall appearance suggests a relatively evolved system with a low ongoing star formation rate.
