The galaxy appears to be undergoing a merger event. There are two distinct, roughly spherical bright concentrations of light, suggestive of galactic nuclei. These components display a yellowish-orange hue, indicative of an older stellar population. A faint, diffuse halo of light surrounds both nuclei, connecting them, indicating possible tidal interactions. The overall structure suggests a relatively smooth morphology, with a notable absence of prominent spiral arms or distinct disk features. There is also a hint of disturbances in the light distribution around the two cores.
