The galaxy appears as a centrally concentrated, smooth object, with a somewhat elliptical morphology. The color profile suggests a redder core region, with bluer hues on the outskirts, hinting at possible differences in stellar populations or dust content between the galaxy's center and its outer regions. No distinct spiral arms or bar structures are discernible, rather a smoothly fading luminosity gradient outwards. There are no signs of strong tidal features or major disturbances, pointing to the system being relatively relaxed and non-interacting, or that any previous interaction was minor. The overall appearance is consistent with a possible elliptical galaxy or a lenticular galaxy seen at a considerable distance.