The galaxy presents as a single, relatively smooth and rounded structure. It exhibits a concentrated central region that is roughly circular in shape. The color profile suggests an older stellar population, with a yellowish-red hue dominating the overall appearance. There is no visible evidence of spiral arms or significant dust lanes. The outer regions of the galaxy appear to fade gradually into the background, indicating a lack of sharp edges or actively star-forming regions. Based on its morphology, it is likely an elliptical galaxy or a lenticular galaxy viewed face-on, with minimal signs of recent mergers or major disturbances.
