The galaxy appears as a smooth, elliptical-like structure. Its light distribution suggests a centrally concentrated morphology, with a gradual decrease in intensity towards the outer regions. There is a slight elongation, but overall the object exhibits a relatively high degree of circular symmetry. The color is primarily yellowish, indicating an older stellar population. Faint wisps or minor disturbances are visible and suggest past or ongoing interactions, but no major merger event is apparent.
