The galaxy presents as a disturbed morphology, potentially indicative of a recent or ongoing merger event. The central region of the galaxy displays a smooth, diffuse component, but there is visible asymmetry. The overall color gradient suggests a complex distribution of stellar populations, possibly with a slightly bluer component concentrated in the disturbed regions. Patches of redder color may indicate either areas of dust extinction or older stellar populations. There also seem to be faint tidal tails present. 
