The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology with a high degree of central concentration. It displays a round shape with minimal deviation from circularity. The color gradient suggests a stellar population that is largely composed of older stars. There is a small amount of star formation. There is no evidence of spiral arms or a significant disk component. Minor disturbances or interactions with other galaxies may be present, but they are not significantly disrupting the overall structure. 
