The galaxy presents as a slightly elongated structure with a smooth light distribution. It exhibits a dominant central bulge that appears roughly symmetrical. There is some evidence of disc-like features, however, it does not contain well-defined spiral arms, based on its smooth appearance. There is a significant amount of light distributed in blue. The blue light and modest inferred star formation rate suggests ongoing, though not intensive, star formation. The galaxy is of modest size, approximately 3 kpc in radius. There is another galaxy in the image, although the two do not appear to be interacting.
