The galaxy presents as a relatively compact and centrally concentrated system. It exhibits an overall elliptical morphology, appearing mostly smooth in texture. The light profile suggests a gradual decline in brightness from the core outwards, showing no distinct spiral arm structure. The color gradient appears to shift from bluish-white in the center to a slightly more reddish-yellow hue in the outer regions, which could indicate a change in stellar population or dust content. There may be some minor tidal disturbances, but the overall structure seems largely undisturbed.
