This galaxy presents a distinct spiral structure with tightly wound arms. These arms are visible, exhibiting a level of star formation activity. The central bulge appears prominent. The galaxy is not observed edge-on; instead, the disk is at an inclination that allows a clear view of the spiral structure. It is likely a two-armed spiral galaxy. It is not undergoing a major merger, although there may be a minor disturbance affecting its shape. Based on the magnitude information, this is a luminous galaxy.
