The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a concentrated, bright, yellowish-white glow, indicative of a high density of older stellar populations. Moving outward from the core, the light gradually diffuses, transitioning into a more greenish hue. The shape of the galaxy is more in between than a perfect circle, but it is not particularly elongated. There is no visual evidence of strong spiral arm structures or bar features. Overall, the galaxy's morphology suggests a quiescent system with a comparatively low rate of star formation. There are no obvious signs of recent or ongoing major mergers or tidal disturbances affecting its overall shape. 
