The galaxy is a spiral type, exhibiting well-defined, tightly wound spiral arms. The arms appear somewhat flocculent in nature, with a high concentration of star formation. The central bulge is prominent and appears to be relatively large. The galaxy's disk is oriented at an angle to our line of sight, indicating it is not a pure face-on galaxy but is only slightly tilted. The galaxy exhibits a subtle bar structure. The galaxy does not appear to be undergoing any major merging or interaction events.