The galaxy presents a predominantly smooth, elliptical morphology. Its light profile appears centrally concentrated, exhibiting a gradual decrease in brightness with increasing radial distance from the core. A subtle color gradient is visible, transitioning from a slightly bluer hue in the outer regions to a yellower, more reddish tone towards the galactic center. The overall structure suggests a relatively evolved system, likely dominated by older stellar populations. There are no apparent signs of strong spiral arm structures, tidal disturbances, or ongoing major merging events. The round shape is largely undisturbed, showing no major distortions.
