The galaxy presents as a spiral with a fairly compact but bright core, suggesting the presence of a significant central bulge. The spiral arms are somewhat flocculent, with a clumpy, discontinuous appearance rather than tightly wound, well-defined structures. These arms exhibit a distinct blue hue, indicating ongoing star formation within. There are brighter, more concentrated regions of blue scattered along the arms, likely corresponding to large clusters of young, hot stars. The galaxy also exhibits signs of tidal disturbances, with irregular morphology in the spiral arms and hints of extended structures that may have formed as a result of interactions with another galaxy.
