The galaxy exhibits a distinct spiral structure, with two prominent arms emanating from a central region. The arms appear relatively well-defined, displaying a moderate winding pattern. The central bulge is not particularly pronounced, appearing small compared to the overall size of the disk. There is some evidence of a bar-like structure traversing the central region, but it does not appear particularly strong. The disk is not viewed edge-on, and there is no obvious dust lane. The overall appearance suggests a disk-dominated galaxy undergoing active star formation in its spiral arms, with indications of possible interaction or minor disturbance within the galactic structure. The galaxy appears to be experiencing no major interactions with other large galaxies, and appears to be in an isolated part of space. 
