The galaxy presents a distinct spiral structure, with a high probability of having two prominent arms. These arms appear loosely wound, extending outwards from a central region. There is a suggestion of a bar-like structure intersecting the central region. The central bulge size looks negligibly small. The likelihood of a minor disturbance is present, but there is nothing major suggesting merging activity is occurring. The colours suggest ongoing star formation, based on the bluer colours in the spiral arms. The galaxy presents as a disk with a generally blue cast, seen at an angle close to face-on.