The galaxy presents a morphology that is neither purely smooth nor a well-defined spiral. It exhibits a central, bright region that diffuses outwards, lacking strong spiral arm structures. Some disturbances can be seen in the structure. The galaxy exhibits a subtle, diffuse halo, suggesting a fairly well-mixed stellar population that is either a somewhat smooth elliptical or a disturbed disk galaxy. The galaxy is of moderate size, and has a moderate rate of star formation.
