The object presents as a merging galaxy system. The morphology suggests a relatively advanced stage of interaction, characterized by multiple distinct, luminous components. The dominant feature appears to be a central concentration of light, likely representing the core of one of the progenitor galaxies. To the southeast there is a second concentration. An additional concentration of light is visible, but is more diffuse. Faint tidal features, possibly plumes or bridges, are visible connecting the various nuclei, indicating ongoing gravitational interaction. Color gradients are present within the system, with the central regions exhibiting a reddish-orange hue and the outer regions displaying a greenish tint. The system is undergoing some star formation, but is dominated by older stellar populations.
