The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. The galaxy appears predominantly featureless, lacking any distinct spiral arm structure or prominent dust lanes. Color gradients suggest a higher concentration of older stellar populations. No signs of active galactic nuclei activity or recent major mergers are clearly discernible from this image. There is only a very slight indication of possible minor disturbance. Its shape is relatively circular, indicating a low degree of ellipticity. 
