This galaxy appears to be a spiral galaxy, viewed at an inclined angle. It displays prominent spiral arms that are somewhat loosely wound. Evidence of active star formation is suggested by the mottled appearance within the arms, indicative of HII regions and young star clusters. A central bulge is apparent, and appears moderate in size. There is evidence of tidal disturbances and possible interactions, exhibited by asymmetric and extended arm structures. The galaxy appears to be undergoing a major merger or experiencing significant gravitational interactions with another galaxy. A bar structure is faintly visible extending through the bulge.
