The galaxy presents as an elliptical morphology. It displays a smooth, concentrated light profile, with the highest intensity toward the center. The galaxy exhibits a subtly elongated shape. The color gradient suggests a redder core, potentially indicative of an older stellar population or dust obscuration. Fainter, bluer regions exist towards the outer edges of the galaxy, possibly signaling some degree of recent star formation activity, albeit at a low rate. There are no apparent signs of tidal disturbances or ongoing mergers visible.
