The galaxy presents as a spiral type, with a disk-like structure inclined at an angle to our line of sight. The spiral arms are well-defined, displaying a moderate to tight winding pattern. The disk appears relatively thin and the arm structures show an average of three arms. The central bulge component appears to be a moderate size. There is no obvious strong bar feature crossing the central region, nor a strong concentration of light toward the nucleus. No major signs of interaction with other galaxies are evident.
