The galaxy presents as an object exhibiting characteristics of a merging system. Two distinct luminosity peaks are observed, one exhibiting a yellowish-orange hue and the other a bluer tone. Morphologically, the system appears disturbed, lacking a clear, defined structure, instead suggesting an ongoing interaction between two galaxies. The overall color profile hints at a population of both older, redder stars and younger, bluer stars, potentially indicating ongoing or recent star formation activity triggered by the merger. There is evidence of tidal features, though subtle, further supporting the merger interpretation. The system is relatively compact, with an estimated diameter of approximately 5 kpc. Overall the galaxy presents as two galaxies in the process of a late stage merger, with the presence of old stellar populations and recent star formation activity. 
