The galaxy presents as an approximately elliptical object. The central region exhibits a brighter, more concentrated luminosity. The color profile suggests a relatively uniform stellar population throughout the majority of the galactic body. There is a slight distortion on one side and an arm extending out from the main disc. The arm has a slightly different color that the main body, suggesting either different ages of stars or a starburst. The color of the disc also suggests that it may be actively forming stars. There are areas of disturbances within the morphology of the galaxy. There is a potential merging event with a smaller object adjacent to the right side of the galaxy, which may explain the visual disturbances within the main morphology.
