This galaxy exhibits a complex morphology suggestive of an ongoing or recent interaction or merger. The galaxy’s central region presents a bright, slightly elongated core. Emanating from this core is a fainter, more diffuse halo. Within the halo, there appears to be evidence of asymmetry and irregularities, including what could be tidal features or distorted arm structures. The overall light distribution seems disturbed, as if two galaxies are colliding, with a merging of the bright galactic centers. The galaxy appears to have an active star forming rate, as seen by the light, and mass. There appear to be possible merging components that are creating a higher disturbance than a normal galaxy. The disk fraction looks low, suggesting a elliptical morphology.
