The galaxy appears to be a spiral galaxy, viewed at an oblique angle, displaying a disk structure with discernible spiral arms. The arms appear somewhat flocculent and extend outwards from a central region. The bluer tones are indicative of active star formation within the spiral arms. The central region is less defined, with no obvious bulge. There is indication of possible interaction or recent merger, given disturbances within the arms. The galaxy displays a moderate amount of internal structure.
