The galaxy presents an elliptical morphology with a smooth, centralized bulge. The central region exhibits a higher intensity, suggesting a concentration of stars or potentially an active galactic nucleus. There is the possibility of a disk component with some apparent disturbances, or a tail of ejected material extending from one side of the galaxy, indicated by a faint greenish blue haze. Redder hues can be seen as a rim around the galaxy. The primary color is a vibrant blue, indicating active star formation or a different emission process. The galaxy appears to be undergoing a minor gravitational interaction with a companion galaxy.
