The galaxy presents a disk-like morphology, with a relatively compact appearance.  Evidence of disturbances in the form of slight asymmetries and irregularities is apparent. The central region shows a somewhat smooth texture.  The disk appears disturbed, possibly indicating a minor or major merging event, however based on the image it is hard to know the exact situation. Overall, the galaxy's morphology hints at potential interactions or recent mergers that are influencing its structure. 
