The galaxy exhibits a complex morphology, suggestive of an ongoing or recent interaction or merger. The primary component appears relatively smooth and rounded, exhibiting a blue-white color, implying a population of younger, hotter stars. A secondary, less prominent component displays a distinctly yellowish-orange hue, possibly indicative of an older stellar population and/or significant dust obscuration. This secondary component is more diffuse and elongated. There is evidence of tidal distortion, with a faint, extended feature that could be a tidal tail or bridge. Overall, the system does not appear to be in a state of equilibrium, exhibiting clear signs of dynamical disturbance.
