The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, though it appears moderately round rather than highly elongated. The central region displays a bright, concentrated core, which likely hosts an actively accreting supermassive black hole. The light profile smoothly decreases from the core outwards. A subtle color gradient is visible; the core appears more yellow-red, with the outer regions exhibiting a bluer hue. There is no evidence of spiral arms or a distinct disk. The structure indicates a possible lack of active star formation. The color indices suggest that the stellar population may be dominated by older, redder stars, with a possibility of some ongoing, low-level star formation in the outer regions as indicated by their slightly bluer color. The overall appearance of the galaxy suggests that it is an early-type galaxy.
