The galaxy presents as a single, relatively smooth object, with a near-spherical morphology. It exhibits a concentrated central region of high luminosity, appearing yellowish-white. The light gradually diminishes with radial distance from the center of the galaxy. There is no clear evidence of spiral arms or a bar structure. The galaxy has a smooth appearance, and there are no obvious signs of recent major merger activity. There appears to be little to no blue light emission, suggesting older stellar populations. The galaxy is not perfectly round but has very slight ellipticity.
