The galaxy presents as a flattened, elongated structure, suggestive of a disk galaxy seen nearly edge-on. The central bulge appears bright and concentrated, fading into a less defined disk. There is evidence of some structure within the disk, although the resolution prevents a clear delineation of spiral arms or dust lanes. The color is generally bluish-white, which potentially indicates the presence of a population of younger, hotter stars, and possibly ongoing star formation within the galaxy. There appear to be no obvious signs of major mergers or strong tidal disturbances, but there is a possible faint extension of the disk material on one side.
