The galaxy appears to be undergoing a significant merger event. There are several distinct luminous clumps, which are possibly tidal tails or remnants of interacting galaxies. The central region appears relatively smooth and somewhat rounded, although it is not perfectly spherical. A plume or extended feature, slightly elongated, extends outward from one of the luminous clumps, exhibiting a redder color. The overall color gradient suggests varying stellar populations, with bluer regions potentially indicating more recent star formation, and redder regions indicating older stellar populations. There is some evidence of a disk-like structure, but it is highly disrupted. There are no clear spiral arm structures.
