The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a central bulge that is brighter and more concentrated. The overall color profile suggests a predominantly older stellar population, with a subtle blue tint. There is a lack of strong spiral arm features or prominent dust lanes. The galaxy shows a slight asymmetry and potential minor disturbances in its outer regions, hinting at possible past interactions or mergers. Overall the galaxy appears to be a relatively normal, undisturbed galaxy. 
