The galaxy exhibits an overall elliptical morphology. The core region is relatively smooth and appears to be dominated by older stellar populations, evidenced by its redder color. Moving outward from the core, a diffuse, greenish halo extends, suggesting the presence of ongoing star formation or a population of younger, hotter stars compared to the core. There is a suggestion of a slight disk-like structure embedded within the broader elliptical form, though this feature is not sharply defined. The overall structure appears relatively undisturbed, without strong signs of recent major merger activity.
