The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Two distinct, tightly wound spiral arms emanate from a bright, yellowish central bulge. The arms display a predominantly bluish hue, suggestive of active star formation regions. The bulge appears relatively small compared to the overall disk size, with an elongated morphology. The spiral arms show some disturbances, hinting at possible past interactions or internal dynamic processes. There is the possibility of a weak bar in the center of the galaxy.
