This galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. Two distinct luminous components are visible, each displaying a relatively smooth, centrally concentrated light distribution. These components show differing colors, with one exhibiting a more yellow tone and the other a whiter color. Evident tidal features, possibly faint stellar streams or diffuse light, appear to connect the two components and extend outwards, further indicating gravitational interaction. The overall shape of the system is elongated, oriented approximately along a northeast-southwest axis. There is potential evidence of disturbance within one of the merging galaxies, showing a non-uniform distribution of light.
