The galaxy exhibits a prominent spiral structure with tightly wound arms emanating from a bright central bulge. The arms are clearly defined, displaying a clumpy morphology indicative of active star formation. Blue hues are observed along the spiral arms, suggesting the presence of young, hot stars. The central bulge appears smooth and yellow, potentially indicating an older stellar population. The disk is relatively large, extending significantly beyond the bulge. There is no apparent bar structure. The galaxy displays a high degree of rotational symmetry.
