The galaxy presents a discernible spiral structure, evidenced by the presence of spiral arms. These arms appear somewhat fragmented and not as tightly wound. The overall morphology suggests an intermediate spiral type. A central bulge is present, although not highly dominant. The disk component is readily apparent. There is no significant central bar feature visible. The galaxy exhibits a non-negligible level of disturbance, possibly indicating an interaction or merger event in its recent history. The color profile suggests ongoing star formation activity within the spiral arms.
