The galaxy exhibits a morphology indicative of a merging system. Two distinct, roughly spherical, components are visible, both displaying a yellowish-orange hue. This color suggests an older stellar population.  A significant tidal interaction is apparent.  The two components may be in the early stages of merging, with considerable mass already concentrated in the centers. There is no clear spiral structure visible. A third, more compact, and distinctly blue object is visible and may be a star-forming region, or possibly a background object. The overall smoothness of the primary components suggests a relatively evolved system, potentially transitioning towards an elliptical morphology as the merger progresses. Overall, the system seems to be experiencing significant disturbances.
