The galaxy presents as a spiral galaxy with a notable disk component. Spiral arms are present, exhibiting a tightly wound morphology across a large portion of the disk. The central bulge is moderately prominent, displaying an intermediate size relative to the overall galaxy. A bar structure is potentially present, but indistinct, possibly classified as weak. There is no obvious major merger activity, although there appears to be a minor disturbance in morphology. The galaxy's orientation is face-on, allowing for a comprehensive view of its spiral structure.
