The galaxy appears as a relatively smooth, elliptical structure, exhibiting a high degree of circularity. There is little indication of spiral arms or significant disk features. The galaxy possesses a centrally concentrated luminosity profile, with a gradual decline in brightness towards its outer regions. Faint color gradients are observable, with the core appearing slightly redder than the surrounding halo. There is no apparent ongoing merger activity or significant tidal disturbances. The object is consistent with a relatively evolved galaxy at a moderate redshift.
