The galaxy presents a predominantly smooth morphology, appearing largely featureless. It exhibits a somewhat elliptical shape, deviating slightly from a perfect sphere. The light profile suggests a centrally concentrated structure with a gradual decrease in luminosity towards the outer regions. Color gradients are subtle, but indicate a bluer core region, suggesting younger stellar populations there. The overall color is skewed towards redder hues, which may indicate an older stellar population or dust obscuration. There is no strong indication of spiral arms or a prominent disk structure. There is also no obvious interaction or merger activity.
