The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, luminous core region that gradually diminishes in intensity outwards. Coloration suggests an aging stellar population, dominated by redder wavelengths. There's minimal indication of active star formation regions, consistent with a galaxy that has largely exhausted its supply of gas and dust. The overall structure suggests a relatively relaxed system with no significant signs of recent or ongoing mergers or tidal disturbances. The shape is tending towards an elliptical, with no distinct features visible.
