The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light distribution exhibits a radial gradient, being brightest towards the core and gradually fading outwards. The central region displays a yellowish hue, potentially indicative of an older stellar population. There is a subtle transition to a bluish-white color in the outer regions. The overall shape is generally round, though with hints of slight elongation. There is no evident spiral structure or significant dust lane obscuration. The object appears undisturbed, with no clear signs of tidal interactions or ongoing mergers.
