The galaxy presents a largely smooth, elliptical morphology. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population, while the outer regions display a bluer tint, indicative of more recent star formation. The overall structure appears largely undisturbed, with no obvious signs of major merging events or significant tidal distortions. A faint, extended halo is suggested by the gradual decrease in light intensity from the core to the periphery. The galaxy is relatively compact, with a noticeable concentration of light towards its center.
