The galaxy presents as a centrally concentrated, relatively smooth object. Its shape is generally elliptical, appearing mostly round with a slight deviation towards an intermediate form. The light distribution indicates a higher concentration of older stellar populations in the core, which fades smoothly outward. Overall, the galaxy appears to be undisturbed, showing no significant signs of recent or ongoing mergers, though there is very faint hint of a possible minor disturbance in the halo. Color gradients suggest a relatively quiescent star formation history. The galaxy is redshifted to a notable degree, suggesting a significant distance from the observer.
