The galaxy appears to be a spiral type, exhibiting a prominent disk structure. The spiral arms are distinct, exhibiting a multi-armed morphology. The winding of the arms ranges from tight to loose across the galaxy, and there's no apparent bar structure. A bulge is present, but not particularly dominant, appearing relatively small compared to the overall disk size. The disk is not seen edge-on. There is no obvious evidence of significant ongoing merger activity or major disturbances, but I can't be sure about minor ones. The galaxy displays colors indicative of ongoing star formation, with a hint of younger stellar populations present within the spiral arms. Overall, it is likely a spiral with a notable disk and identifiable structure.
