This galaxy exhibits a distinct disk-like structure, viewed at an intermediate angle, neither fully face-on nor edge-on. Spiral arms appear present, though somewhat flocculent and not tightly wound. These arms are subtly blueish, which suggests ongoing star formation. The central bulge is not very prominent, appearing rather small relative to the overall size of the disk. There isn't evidence of a strong bar-like structure bisecting the nucleus. The morphology indicates the presence of a minor disturbance or possible interaction, shown through the clumpy nature of the spiral arms. Overall, the galaxy appears relatively faint with a moderate level of star formation activity, without a substantial bulge and is showing possible signs of merging.
