The galaxy presents as a system showing signs of tidal disruption. It features a central, brighter core exhibiting a relatively smooth morphology, transitioning to a more disturbed structure at the edges. One part of the galaxy is elongated, cigar shaped and has a reddish color, suggesting an older stellar population and/or significant dust obscuration. The other part is smoother and bluer in color, implying a region of ongoing star formation. The presence of disturbed features, particularly the asymmetry and apparent tidal tails or bridges, implies the possibility of a recent or ongoing merger event.
