The galaxy presents as a luminous, centrally concentrated object with a smooth overall morphology. It appears to be elliptical in shape, exhibiting an approximate aspect ratio of 1:1 with slightly blurred edges. The core displays a bright, yellowish-white hue, indicative of an older stellar population. There is a slight color gradient, transitioning to a redder and fainter halo or extended component surrounding the brighter core. No distinct spiral arms or dust lanes are discernible within the galaxy's structure. Faint disturbances are visible and potentially indicative of a merger.
