The galaxy appears as a singular, relatively symmetrical luminous object. Its overall morphology suggests a generally smooth, elliptical shape, with a lack of prominent spiral arms or a clearly defined galactic disk. There is a slight elongation, though the deviation from perfect circularity is not extreme. No major disturbances or obvious signs of ongoing mergers with other galaxies are apparent in this image, although there might be subtle indications of minor tidal interactions on the outskirts of the visible structure. The light profile suggests a gradual dimming from the center outwards with no obvious bright clumps. 
