The galaxy presents as a spiral type, observed at a slight angle to face-on. The disk component is prominent, exhibiting a notable degree of structure. Spiral arms are readily discernible, with the majority appearing tightly wound around the galactic center. The arms show a flocculent nature, with distinct regions of star formation indicated by bluish hues along the arm structures. The central bulge appears moderate in size relative to the disk, showing a yellow-red color, suggesting an older stellar population. No strong bar feature is apparent across the central region. Overall, the disk exhibits features suggesting that it is relatively undisturbed, without substantial signs of a major merging event.
