This galaxy appears to be a spiral galaxy, viewed at a significant angle. The central bulge is relatively bright and elongated along the major axis of the galaxy, exhibiting a smooth, diffuse light distribution. The spiral arms are not sharply defined, appearing somewhat flocculent. Their color suggests they are actively forming stars. The galaxy's overall color is bluish, although the arms display a more prominent blue hue, indicative of younger stellar populations. The galaxy’s shape is consistent with a disk-like structure seen nearly edge-on. There is no strong evidence of ongoing major mergers, though a minor disturbance cannot be ruled out.