The galaxy presents as a face-on spiral structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. Two distinct spiral arms emanate from the central region, exhibiting a tightly wound morphology. These arms appear asymmetric, indicating possible interactions or disturbances. The spiral arms show variations in color, with patches of blue hinting at regions of active star formation. There is a hint of a possible bar structure within the central region, although not distinctly prominent. The overall appearance indicates a relatively massive galaxy undergoing active star formation, but without any significant signs of tidal disruption or major merger events.
