This galaxy presents as a spiral, seen at an oblique angle. Prominent spiral arms are visible, extending from a central bulge region. The bulge appears relatively moderate in size. There is some indication of a bar-like structure extending across the bulge, though it's not sharply defined. The spiral arms show distinct regions of star formation. The galaxy does show some evidence of a possible interaction or disturbance event; there is some irregularity observed in the spiral arm structure, as well as some disturbances in the outer disk. There is some light that indicates star formation is currently active.
