The galaxy appears to be a spiral type, exhibiting a distinct disk structure viewed at a slight angle. The central bulge is somewhat prominent but not dominant. The spiral arms are clearly visible, winding outwards from the central region. Star formation is evident throughout the disk, indicated by bluer regions associated with younger stars and nebulae, particularly concentrated along the spiral arms. The overall color suggests a mix of stellar populations, with a more yellowish central bulge possibly indicating older, less active star formation. The galaxy does not show obvious signs of major merging activity, though some minor disturbances might be present in the outer regions of the disk. Overall, the galaxy presents as a relatively undisturbed spiral system with ongoing star formation within its disk.