The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent merger event. Two distinct nuclei are visible, indicating the presence of two interacting galaxies. The system appears to have a somewhat irregular shape, with tidal features or extended stellar halos potentially resulting from gravitational interactions. The galaxy displays a color gradient, with the central regions appearing reddish and the outer regions showing bluer tones. This could indicate a difference in stellar populations, with older, redder stars concentrated in the center and younger, bluer stars in the periphery, possibly triggered by the merger. Some dust lanes are visible, further obscuring light and hinting at ongoing star formation activity. Overall, the galaxy presents as a system undergoing dynamic evolution, influenced by gravitational interactions and the resulting impact on star formation and morphology.
