The galaxy exhibits an overall elliptical morphology, appearing elongated or cigar-shaped in its orientation. The light distribution is centrally concentrated, with a smooth, diffuse appearance indicating a lack of prominent spiral arm structures. The galaxy core is relatively bright. There are hints of bluer hues along the outer edges of the galaxy. The smoothness suggests a population dominated by older stars, though some recent star formation may be present. The lack of significant tidal features or irregular shapes suggests it is not currently undergoing a major merger event, although a minor disturbance cannot be ruled out. The overall structure implies that the galaxy is relatively undisturbed and relaxed, suggesting a more evolved system.
