The galaxy presents a disk-dominated morphology with prominent spiral arm structures. These arms are loosely wound, extending outwards from a central bulge that appears relatively small. A bar-like structure seems to bisect the bulge region. Evidence of active star formation is suggested by the overall blue hue of the disk, with the arms showing slight variations in color intensity. It is likely undergoing some merging or tidal interaction, with its disk appearing slightly perturbed. The dust lanes within the spiral arms are not sharply defined, indicating a flocculent structure.
