The galaxy appears as a relatively compact object, exhibiting a smooth, elliptical morphology. Its light profile suggests a centrally concentrated brightness, gradually fading towards the outer regions, indicating it is more likely an elliptical galaxy. There is a distinct color gradient, with the central bulge appearing more yellowish, possibly indicative of an older stellar population. No spiral arm structures or prominent dust lanes are discernible in this image. Its overall shape is quite round. There is no evidence to suggest major disturbances due to galactic mergers, though minor disturbances or tidal features cannot be completely ruled out at this resolution. 
