The galaxy presents a primarily smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, suggesting a high stellar density. Surrounding the core, the galaxy displays a diffuse halo. This halo shows a gradual decrease in luminosity from the inner regions outward. The overall color of the galaxy appears to be leaning towards the redder end of the spectrum. There are no prominent spiral arm structures visible. There may be a hint of subtle dust lanes or irregularities in the outer regions, but these features are not distinctly defined. There is no strong evidence of recent or ongoing major merger activity.
