The galaxy exhibits a complex morphology suggestive of an ongoing or recent interaction. Two distinct components are visually apparent. One component presents as a somewhat amorphous structure with a diffuse halo. The color is relatively uniform, with a slight central brightening. The second component is compact and appears bluer in color. The light distribution is uneven with a lumpy structure. There appears to be a connecting bridge of material between the two components, indicating possible tidal interactions. There is also evidence of a more diffuse stellar envelope extending around the galaxy, which could be tidal debris. Overall the morphology is disturbed and suggestive of a merger event.
