This galaxy appears to be a spiral type, exhibiting prominent spiral arms extending from a somewhat indistinct central bulge region. The arms display a relatively loose winding pattern, suggesting a flocculent or grand design spiral structure. The bluer hues concentrated within the spiral arms are indicative of ongoing star formation, implying the presence of young, hot, massive stars. There is evidence of a bar-like structure traversing the galactic center, although it is not particularly pronounced. The overall structure of the galaxy indicates it may be undergoing some form of interaction or disturbance, possibly a minor merger, given the asymmetry and irregularities observed in its morphology. The galaxy shows a relatively low fraction of light concentrated in a smooth bulge.
