The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology with high degree of roundness. There is no obvious disk structure visible; it appears to be a spheroidal system, possibly an elliptical galaxy. A slight color gradient is observable, with a more reddish core transitioning to a bluer outer halo. The galaxy shows no signs of a major ongoing merger, although minor disturbances or interactions cannot be ruled out based on this single image. The object's half-light radius is a few kiloparsecs, suggesting it is a galaxy of considerable size. The overall luminosity indicates it is a fairly luminous system. The color suggests a relatively evolved stellar population, though some ongoing star formation may be present.
