The galaxy exhibits a clear spiral structure. The spiral arms appear well-defined, extending outwards from a central bulge. There is a suggestion of a bar-like structure across the central region. The bulge appears moderate in size relative to the overall galactic disk. The color distribution within the galaxy indicates some active star formation. Patches of bluer light are observed within the spiral arms, suggestive of younger, hotter stars. The overall appearance suggests a galaxy that is relatively undisturbed, with no obvious signs of a major ongoing merger, though there is a potential for minor disturbances.
