The galaxy presents as a relatively smooth, concentrated structure. The color gradient suggests a population of older stars, concentrated towards the center. There is also a greenish-blueish tint that forms a diffuse region around it, which could suggest ongoing, but minimal, star formation or potentially the presence of an active galactic nucleus obscured by dust. The roundness of the central light suggests it is likely an elliptical galaxy. There are no obvious signs of spiral arms or a central bar. No major interactions or mergers are apparent in this image, although there may be minor disturbances. The overall form suggests that the system is relatively relaxed and mature.
