The galaxy appears to be a merging system, composed of two distinct galactic nuclei embedded within a diffuse halo of starlight. Each nucleus exhibits a bright, concentrated core, indicative of a high concentration of stars. The overall morphology suggests an elliptical or lenticular galaxy type, although the ongoing merger could be disrupting any pre-existing spiral structure. The outer regions of the galaxy are faint and somewhat irregular in shape, possibly due to tidal interactions between the two galaxies. The color profile suggests a population of older stars, with some redder hues visible, but there is also evidence of bluer regions, particularly in the outer halo, hinting at more recent star formation activity, maybe as a result of the merger event.
