The galaxy appears as a relatively smooth, elliptical-like structure. Its morphology is dominated by a central bulge that is somewhat round. There is a distinct color gradient moving from the center of the galaxy outward. The central region exhibits a reddish hue, transitioning to greenish-blue in the outer regions. The gradient is indicative of differing stellar populations. Based on the smoothness of the galaxy, it does not appear to be undergoing any significant merging activity or major disturbances. 
