The galaxy appears to exhibit a merging or interacting morphology. Multiple galactic nuclei are suspected, with evidence of tidal distortion present in the diffuse light distribution. The overall shape can be described as elongated, with an axis ratio suggestive of a disk-like component viewed at an oblique angle. The light profile appears relatively smooth in some regions but shows irregularity in others, indicating active star formation is possible. The galaxy's color suggests a mix of stellar populations, with some bluer regions indicative of ongoing star formation and redder regions indicative of older, more evolved stars. The galaxy is quite luminous, emitting a significant amount of light in the observed bandpasses. There is a hint of disturbance suggesting possible tidal tails extending outward.
