The galaxy presents as a relatively smooth, elliptical-like structure. Its color is predominantly yellow/orange, suggesting a population of older stars and a diminished rate of current star formation. There is a bright central region that likely indicates a concentration of stars near the galactic nucleus, and possibly the presence of a supermassive black hole. No spiral arms or significant dust lanes are visibly discernible. The overall appearance suggests a galaxy that has largely exhausted its supply of gas and dust, resulting in a more quiescent and evolved stellar population. There may be some evidence of a very minor disturbance visible, but it is hard to say from the image alone.
