The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. The central region exhibits a bright, yellowish-white luminosity, indicative of a high concentration of older stellar populations. Extending outward from the core, the galaxy displays a more diffuse and less structured halo. There is a slight elongation in the galaxy's overall shape, suggesting it is not perfectly spherical. There might be some subtle hints of spiral structure, but the smoothness dominates the visual impression. There is a second object to the bottom left of the galaxy. The galaxy does not appear to be undergoing a major merger, however some smaller disturbances cannot be ruled out. The galaxy displays a mix of light indicating some on-going star formation activity.
