The galaxy presents as a relatively smooth, elliptical morphology. There are no prominent spiral arms or a central bar apparent. The color gradient indicates a concentration of older stellar populations towards the core, which appears yellowish-orange. The outer regions display a bluer hue, which might indicate ongoing, though subdued, star formation. The galaxy does not appear to be undergoing any major merging events or tidal disturbances, although there is the possibility of minor disturbances. Overall, this galaxy seems to be a relatively undisturbed system.
