This galaxy presents an elliptical morphology, appearing relatively smooth and somewhat elongated. The central region exhibits a bright, concentrated core, suggesting a higher stellar density. Progressing outwards, the galaxy gradually fades into a diffuse halo. There may be some spiral structure but that's hard to tell. Some minor disturbances possibly could be seen, likely indicative of minor interactions or past merger events.
Overall, the galaxy seems relatively undisturbed and quiescent.
