The galaxy presents as a spiral structure, exhibiting flocculent arms. These spiral arms appear to be composed of a mixture of diffuse, lower-surface-brightness regions, as well as some tightly wound sections, possibly indicating varying stages of star formation and gas density. The central bulge is moderately prominent. While there is no obvious bar, a slight elongation or asymmetry is suspected in the nuclear region which hints at a weak bar. Evidence of minor tidal disturbances are present, potentially the result of an ongoing or recent interaction, possibly with a smaller dwarf galaxy. The overall color is a yellowish-white, suggesting an evolved stellar population, though the spiral arms have some bluer spots which are likely regions of active star formation.
