The galaxy presents as a smooth, elliptical-like structure, with a noticeable concentration of light towards the center. The core appears yellowish-white, suggesting a population of older stars. Moving outwards from the core, the light gradually diffuses into a more reddish-orange hue. There is little evidence of distinct spiral arms or significant dust lanes within this system from this imaging. The overall symmetry of the light distribution indicates a relaxed morphology. There may be a slight flattening, resulting in a more spheroidal shape, though it is difficult to fully resolve at this imaging scale.
