The galaxy appears as a concentrated, elliptical-like form with a smooth luminosity profile. There is a distinct central bulge that emits a significant amount of light, transitioning smoothly into the outer regions. The lack of discernible spiral arm structures or dust lanes indicates that the galaxy is relatively evolved and possibly quiescent. There is a slight color gradient, transitioning from a relatively bluer inner region to a redder exterior, suggesting an older stellar population in the outer parts of the galaxy. There are no obvious signs of recent star formation, and the overall morphology implies a relatively relaxed, undisturbed system. There might be some minor tidal disturbance on the right, and bottom of the galaxy, although these could be artifacts. It is highly rounded in appearance.
