The galaxy appears to be a spiral galaxy, exhibiting prominent, well-defined spiral arms. These arms are traced by regions of active star formation, as evidenced by their bluish coloration. There are no obvious signs of major recent mergers or strong tidal disturbances. The central bulge appears relatively small. A faint bar structure is visible. There appears to be a slight asymmetry within the disk, but there is no evidence of edge-on inclination. The galaxy has an overall blue-shifted color, indicating ongoing star formation activity, and is resolved as more of a disk-like structure than smooth or elliptical. The overall morphology suggests a late-type spiral galaxy.
