The galaxy presents a distinct disk-like morphology, viewed at an angle that suggests it is nearly face-on. Spiral arm structures appear present, though moderately defined. These arms exhibit a somewhat flocculent nature. The central bulge is prominent and appears moderate in size relative to the overall disk, with a noticeable concentration of older stellar populations as indicated by the yellowish hue. There's evidence of a bar-like structure traversing the central region. The disk shows areas of bluer light, suggesting star forming regions. The overall structure looks undisturbed, showing no signs of any major ongoing merger events.
