The galaxy presents as a binary system, possibly in the early stages of a merger. Both components exhibit a relatively smooth morphology, with minimal visible dust lanes or spiral arm structures. The color index suggests an older stellar population, leaning towards a redder hue, which is consistent with a lower star formation rate. The shape appears elongated, deviating significantly from a perfect circle, supporting the potential interaction between the two galactic components. Overall, the galaxy appears to be composed of two relatively massive, elliptical-like galaxies, exhibiting characteristics typical of galaxies at redshift z ~ 0.33.