The galaxy appears to be a spiral galaxy, observed at a slight angle relative to face-on. Prominent spiral arms are visible, exhibiting a structure with clear signs of active star formation. The winding of these arms ranges from medium to loosely defined. The galactic bulge is clearly visible, and relatively moderate in size, with a bar that appears relatively strong. The galaxy displays a disk-like structure. The overall appearance suggests the galaxy may be undergoing some level of gravitational interaction or disturbance.
