The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a bright, concentrated core indicative of a significant stellar density, potentially harboring a supermassive black hole. Moving outward from the core, a gradual decrease in luminosity is observed, though the light appears to be fairly even across the galaxy. A subtle blue hue can be seen around the core. It is generally featureless with no pronounced spiral arm structure visible in the image. There might be a slight distortion in the galaxy's shape, but it is difficult to discern.
