The galaxy presents as a system of at least three distinct, bright components within a diffuse halo. These components appear spheroidal in shape and display a yellowish hue, suggestive of an older stellar population. Evidence of interactions is visible, including tidal tails and bridges between the components. This indicates a possible ongoing merger or recent interaction. The overall structure exhibits a smooth appearance, with a high degree of central concentration. Based on morphology, it appears that there is little active star formation, with the majority of the stellar population being older. Overall, a merging galaxy system containing old stars with a considerable mass.
