The galaxy presents as a spiral type, exhibiting a generally face-on orientation. The spiral arms are prominent but somewhat patchy in appearance, and two arms appear to be dominant. Their winding appears to be intermediate, neither tightly wound nor particularly loose. The galactic bulge is moderate in size, not overwhelmingly dominant yet not negligible. The overall impression is one of a galaxy undergoing significant star formation, as suggested by the blue hue within the arms. There is no obvious bar structure. There is a slight asymmetry with an irregular shape, hinting at a possible minor interaction or merging event in its past. The overall morphology does not indicate a system undergoing a major disruptive merger.
