The galaxy presents a flattened, elliptical morphology. There is a noticeable central bulge that appears bright and concentrated. The outer regions of the galaxy exhibit a smoother, more diffuse appearance, fading gradually into the background. Color gradients are present, with the central bulge displaying a slightly redder hue compared to the disk, which shows hints of bluer color. There's no clear evidence of spiral arm structure, though the outer disk does show some slight disturbances, such as a faint tidal tail, which might be interacting with smaller galaxies nearby. Overall, the galaxy seems well-defined, though the faintness of the outer regions suggests it is relatively far away from our point of view.
