The galaxy presents as a spiral galaxy, characterized by a central bulge and discernible spiral arms. The central bulge appears moderately bright with a yellowish hue, suggesting an older stellar population. Two distinct spiral arms emanate from the central region, exhibiting a relatively tightly wound morphology. The arms show clumpy structures, indicative of active star formation regions. The overall color of the arms is bluer than the bulge, supporting the presence of younger, hotter stars within these regions. There is evidence of a weak bar structure present in the central region. The disk of the galaxy is observed face-on, allowing for a clear view of the spiral arm structure. There are no obvious signs of any major merging event currently occurring. The image suggests a relatively massive galaxy with ongoing star formation.
