The object appears to be a spiral galaxy, exhibiting a disk-like structure. There are loosely defined spiral arms. A central bulge is discernible, though appears to be moderate in size, not dominating the overall structure. There is evidence of on-going star formation, indicated by the presence of blue hues along the spiral arms and within the disk. There is no strong central bar feature across the galaxy. There may be some distortion in the morphology, potentially indicative of a minor interaction or disturbance.
