The galaxy presents a largely smooth morphology. The shape is overwhelmingly round. There is a very faint disk component, although most of the light appears to come from a central bulge. This bulge exhibits a yellow-orange hue, indicative of older stellar populations. The surrounding halo of the galaxy shows an irregular distribution of colors, primarily composed of older stars. There are no obvious signs of recent major merger activity. The galaxy shows a low amount of star formation activity.
