The galaxy exhibits a complex morphology suggestive of an ongoing merger event. It displays a primarily smooth central structure, but with clear indications of tidal disturbances. There appear to be multiple components involved.

One component has a somewhat spherical and yellow-orange central region that fades into a soft halo. The other component is noticeably bluer and exhibits signs of ongoing star formation, with a more irregular structure than the first component. Patches of brighter, bluer light are present along with regions where material from the two bodies appears to overlap. Faint, extended features, possibly tidal tails, are visible, though they are not sharply defined. Overall, the galaxy presents as somewhat asymmetric in its distribution of light and morphology.
