The observed galaxy exhibits a spiral morphology, characterized by a central bulge and prominent spiral arms. The bulge appears relatively small, not dominating the overall structure. Two distinct spiral arms emanate from the central region, displaying a moderately wound structure. These arms present as regions of enhanced blue emission, suggesting active star formation. The galaxy's disk is oriented at a shallow angle to our line of sight. Indications are present of disturbances within the spiral arms. The galaxy does not seem to be undergoing any major merging activity. 
