This galaxy appears to be a merging system, exhibiting signs of significant tidal disturbance. The morphology indicates a primary, relatively smooth component with an elongated, cigar-shaped form. A second distinct component shows signs of interaction with the primary galaxy and exhibits bluer light, possibly associated with more recent star formation. The primary component has an orange tint, which suggests an older stellar population. There are clear signs of tidal distortion, with a faint bridge of light possibly connecting the two components, or a potential tidal tail extending from the primary galaxy. Overall, this galaxy presents as an interacting system undergoing a dynamic evolutionary stage.
