The galaxy presents a predominantly smooth morphology. Its overall shape appears largely circular, with only a slight deviation from perfect roundness. There is no prominent central bulge or spiral arm structure discernible in the imagery. The light distribution is fairly homogenous, with a gradual fall-off in brightness from the center towards the outer edges. 

The galaxy exhibits a color gradient, with a bluish tinge in some areas and a more reddish/yellowish hue in others. These color variations potentially indicate differing stellar populations or dust content within the galaxy. While the primary structure seems intact, there's a subtle hint of minor distortion or possible interaction in its appearance, possibly suggesting past or ongoing gravitational interactions with other celestial bodies. There are no indications of major disturbances like tidal tails or very bright star forming regions.
