The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a generally round morphology, with minimal visual disturbances suggestive of recent or ongoing mergers. The galaxy's light profile appears concentrated towards the center, suggesting an older stellar population with little ongoing star formation, with an estimated mass around 10^10 solar masses. The bluer color indicates a higher rate of star formation. The general evenness of its light across the image further confirms the galaxy's status as a relatively unperturbed system. 
