The galaxy appears to be a smooth, elliptical-like structure with a high degree of central concentration. It exhibits a relatively symmetrical, somewhat oval shape. There's a notable difference in color between the central region and the outer edges of the galaxy. The core is a pale bluish green, suggesting possible ongoing star formation or a population of hot, young stars. The outer regions fade into a more diffuse green hue. There are no apparent spiral arms or obvious dust lanes visible. The overall structure seems undisturbed, with no obvious signs of a major ongoing merger. There is a small hint of possible minor disturbance in the very diffuse outer regions.