The galaxy presents as a relatively smooth, concentrated object. It appears elliptical in shape, elongated along one axis. A central bulge is readily apparent, exhibiting a bright yellowish hue, which may indicate an older stellar population or a significant dust component. There is a subtle radial gradient in color, transitioning from a brighter yellow core to a slightly redder halo. No distinct spiral arms or other significant features are immediately discernible. There are no obvious signs of a major ongoing merger or significant tidal disturbances. The galaxy displays a high degree of symmetry. 
