The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid with a gradual decrease in brightness towards the outer regions. The core appears bright and unresolved, indicating a high stellar density. There is a subtle color gradient visible, with the central region exhibiting a slightly bluer hue compared to the redder outer halo. No distinct spiral arm structure or dust lanes are discernible. There is a small but discernible asymmetry, possibly indicating a past minor merger event or tidal interaction, but no major disturbances are apparent.
