The galaxy presents a roughly elliptical morphology, appearing largely smooth in structure. The central region exhibits a concentrated luminosity, transitioning to a gradual decrease in intensity towards the outer edges. The galaxy appears to be generally rounded, with a subtle elongation along one axis. There is a suggestion of disk features or minor disturbances that are hard to see due to distance. Color gradients suggest a diverse stellar population with areas of active star formation present. The overall appearance indicates a mature system with some ongoing stellar activity.
