The galaxy presents a predominantly smooth appearance, exhibiting a somewhat elliptical morphology. The galaxy's overall color profile suggests a higher concentration of older stellar populations, giving it a yellowish hue. There is a slight hint of bluer regions towards the edges, suggesting a possibility of some ongoing, albeit subdued, star formation activity. The galaxy does not display any prominent spiral arms or distinct features typically associated with disk galaxies. No significant signs of major mergers or tidal disturbances are readily apparent, although minor interactions or subtle internal structures cannot be ruled out with this image alone. The galaxy's light distribution seems relatively concentrated towards the center, with a gradual decrease in brightness towards the outskirts.
