The galaxy appears to be a relatively smooth, elliptical or lenticular system. There is a centrally concentrated region of high luminosity, with a gradual decrease in brightness towards the outer regions. The shape is mostly rounded but slightly elongated. There is no obvious spiral arm structure or prominent dust lanes visible in this image, indicating either a lack of significant recent star formation or obscuration of such features. Faint hints of possible tidal disturbances or minor interactions are present in the very outer regions. The galaxy exhibits a blue-ish white hue in the center, transitioning to more reddish colors in the outer reaches. This might indicate a difference in stellar populations, with younger, hotter stars being more concentrated towards the center and older, cooler stars being more distributed in the outer regions.
