The object appears to be a spiral galaxy viewed at a moderate inclination. The central bulge region exhibits a smooth, relatively featureless morphology with a high surface brightness, indicating a concentration of older stellar populations. Moving outwards from the core, a disk structure is visible, though its arm structure is not well-defined. There appear to be some indications of slight disturbances in the disk, which are not immediately identifiable as an ongoing merger. The disk appears largely homogeneous. The object has significant blue light, indicating the presence of younger, hotter stars in its disk.
