The object appears to be a galaxy exhibiting signs of a possible merger or interaction. It presents a somewhat irregular morphology, deviating from a purely elliptical or spiral structure. The galaxy's light profile shows a central concentration, with a smoother, more diffuse halo surrounding it. There are two distinct bright cores, suggesting the potential ongoing merger of two galactic nuclei. The color distribution reveals a dominant yellowish-white hue in the central regions, potentially indicating an older stellar population, while there's a hint of redder tones in a more distinct core, possibly indicating ongoing star formation that is more recent. Overall, this galaxy demonstrates a complex structure characteristic of galaxies undergoing dynamic processes.
