The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are well-defined and tightly wound around a central bulge. The bulge appears relatively small compared to the overall disk size. The color distribution indicates active star formation within the spiral arms, contributing to a bluer hue, while the central bulge shows a more yellow/red hue. The disk is not perfectly face-on, exhibiting a slight inclination. There is no obvious sign of a bar structure. No major interactions or mergers are evident, however, some minor disturbances may be present. The overall form appears well-defined.
