The galaxy presents as a system in the late stages of a merger. Two distinct luminous cores are visible, embedded within a more diffuse, ellipsoidal halo of light. The overall morphology suggests a system that is relatively smooth, with a high degree of central concentration in each of the two cores. There is an absence of well-defined spiral arms or significant dust lanes, suggesting the progenitors of the galaxy may have been ellipticals, or that any spiral structure has been significantly disrupted by the ongoing merger. There is limited evidence of tidal tails or other extended features, indicating a dynamically relaxed system post-coalescence. The color profile appears relatively uniform across the galaxy, with a somewhat redder, slightly old stellar population. There are no prominent blue star-forming regions visible.
