The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. These arms are not tightly wound, instead displaying a more open, somewhat grand design structure. The arms appear slightly patchy, possibly indicating areas of active star formation. The central bulge is small relative to the disk, with a subtle bar-like feature appearing to cross it. The galaxy is inclined at a moderate angle to our line of sight, providing a clear view of the spiral structure. There are signs of possible interactions or disturbances with another galaxy.
