The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population and possibly a supermassive black hole. The light gradually diffuses outward from the core, transitioning into a slightly redder and less intense glow in the outer regions. There is a small reddish blur extending from the galaxy, this could be a tidal tail or a distant object. There is no evidence of spiral arms or significant dust lanes. The overall appearance suggests a galaxy in a relatively advanced stage of its evolution, exhibiting little current star formation. The galaxy appears isolated, with no obvious signs of major interactions or mergers.
