This galaxy exhibits a clear spiral structure, with prominent, well-defined arms. The arms appear somewhat flocculent, displaying a patchy distribution of star formation regions. A slight asymmetry is observed in the arm structure, suggesting possible gravitational interactions. There seems to be ongoing or recent merger activity that is currently resulting in a major disturbance within the structure of the galaxy. The central bulge is moderate in size, with a relatively high degree of central concentration. There seems to be a weak bar feature present within the galaxy's central region. The inclination angle is moderate, neither face-on nor edge-on. The galaxy shows a color gradient, with bluer regions corresponding to areas of active star formation and redder regions indicating older stellar populations.
