The galaxy presents a largely smooth, elliptical appearance with a generally round morphology. A slight asymmetry or possible tidal feature is suggested by a subtle extension or disturbance of the galaxy's isophotes on one side. This could indicate a minor interaction or recent merger event, though the primary structure remains relatively undisturbed. Color gradients suggest a concentration of older stellar populations in the central regions, with possibly slightly younger populations in the extended regions of the disturbance.
