The galaxy presents as a spiral type, exhibiting a defined disk structure. Two prominent spiral arms are visible, tightly wound around the galactic center. A small, faint bulge is observed. The spiral arms display clumpy regions, possibly indicative of active star formation. Evidence suggests the presence of a weak bar feature. No obvious signs of significant tidal distortion or interaction with other galaxies are apparent, though minor disturbances cannot be ruled out. The galaxy shows a relatively smooth morphology with some internal structure within the disk.
