The galaxy presents an overall elliptical morphology, appearing flattened. It exhibits a smooth, diffuse light distribution with a centrally concentrated bulge that fades outwards. There is a slight hint of a possible disk structure, but it is not prominently defined. The color gradients suggest a younger stellar population may exist within the inner regions of the galaxy. There's no indication of a major ongoing merger or strong tidal features, though subtle asymmetries might indicate minor disturbances. It appears to be an isolated galaxy, with no prominent companions nearby.
