The galaxy presents as a system undergoing a merger event, with two distinct components visibly interacting. The upper component appears relatively smooth and rounded, with a concentrated central region exhibiting a whitish hue. The lower component is also rounded, but displays a color gradient shifting from reddish tones at the core to yellower and greener tones at the exterior.

Evidence of tidal disruption is present, but not strongly apparent. While the two components are readily identifiable as separate entities, there is a slight asymmetry in their arrangement, indicative of gravitational interaction. The overall structure does not show significant elongated features beyond those typical of interacting galaxies.
