The galaxy presents as a system undergoing a significant interaction or merger event. There are two primary, somewhat amorphous, components of the galaxy that are visibly merging. These components exhibit a yellowish-red hue, suggestive of an older stellar population with lower levels of on-going star formation. There are no distinctly blue regions indicating recent star formation within this galaxy. The morphological disruption suggests a late-stage merger, with the two progenitor galaxies already largely coalesced. There also appears to be a tidal tail extending from the main body, which is evidence of this merger. The overall structure is complex, lacking a clear spiral or elliptical morphology due to the ongoing interaction.
