This galaxy appears to be in the process of merging. The system presents an elongated morphology with a distinct double nucleus. The primary nucleus exhibits a yellowish hue, suggesting an older stellar population, whereas the secondary nucleus displays a bluer color, possibly indicating more recent star formation. There is evidence of tidal features in the form of faint, diffuse extensions around the main body of the galaxy, most likely due to gravitational interactions. Overall, the galaxy shows signs of significant disturbance, deviating from a regular elliptical or spiral form.
