The galaxy presents as a spiral type, though the spiral arms appear somewhat flocculent. The overall color is bluish, suggesting a relatively young stellar population and ongoing star formation. There appears to be a central bulge, moderate in size, and generally smooth in appearance. There is no evidence of a strong bar structure. No major mergers or tidal disturbances are evident, though some minor irregularities in the outer disk are subtle, and might suggest a possible minor interaction or disturbance.
