The galaxy presents as an elliptical morphology with a smooth, concentrated luminosity profile. Its core exhibits a yellowish-white hue, suggesting a significant population of older stars and a diminished rate of active star formation. The absence of prominent spiral arms or dust lanes reinforces the classification as an elliptical galaxy. There is an observed colour gradient from the core towards the outer regions, transitioning to a more reddish tinge. The overall structure appears largely undisturbed, lacking any obvious signs of recent major mergers, although a hint of asymmetry cannot be ruled out.
