The galaxy presents as a spiral galaxy exhibiting a relatively face-on orientation. A prominent, centrally located bulge with a moderate size is observed. The spiral arms appear well-defined and relatively tightly wound, suggesting a Sa or Sb morphological type. There is evidence of ongoing star formation within the spiral arms, indicated by their bluer color. The dust lanes appear visible, partially obscuring some sections of the spiral arms. The galaxy shows three clearly distinguishable spiral arms. There is no apparent strong bar structure present. No major disturbances or indications of an ongoing or recent major merger event are observed, although subtle asymmetry might suggest a minor interaction. The galaxy exhibits a moderate level of inclination.
