The galaxy presents as a flattened, elliptical shape. The central region is a bright, concentrated bulge, exhibiting a bluish-white hue. This suggests a population of hotter, younger stars in that region. Extending outwards from the central bulge, the light appears more diffuse, with a transition towards reddish hues on the edges. The overall impression is that of a relatively smooth, undisturbed system, possibly in transition between a disk and elliptical galaxy. There are likely stellar populations and dust distributed within the galaxy, creating the change in color observed from blue to red across its radius. There might be minor disturbance in the structure of the galaxy.
