The galaxy presents as a spiral type, exhibiting a discernible disk structure. Spiral arms are prominent, appearing tightly wound around a central bulge. The bulge appears relatively small compared to the overall disk size. The overall shape appears relatively undisturbed, showing no obvious signs of a major merger, however, there may be some minor disturbances. There is evidence of active star formation, indicated by the presence of bluer regions within the spiral arms. A bar structure may be present, but it is not prominent. A significant amount of the disk shows signs of having spiral arms, but it's difficult to say exactly how many arms the galaxy has.
