The galaxy presents a morphology indicative of an ongoing or recent merger. The overall structure is disturbed, exhibiting a departure from a regular elliptical or spiral form. Two distinct, bright nuclei are visible, suggesting the presence of two progenitor galaxies in the process of coalescence.

The light profile appears relatively smooth, with a dominant yellowish-orange color. This color suggests an older stellar population is present, with relatively low ongoing star formation. Faint tidal features, such as wisps or extended halos, can be observed indicating gravitational interactions. Given the prominence of the nuclei and the relative smoothness of the light, this could be an intermediate stage merger, well on its way to full coalescence, with the system approaching a more relaxed elliptical morphology. The overall size appears moderately large, consistent with a massive galaxy system.
