The galaxy presents a morphology consistent with a system undergoing a significant merger event. It exhibits a complex, disturbed structure, appearing elongated with evidence of tidal features. The main body displays a primarily smooth light distribution, with an overall elliptical shape. A secondary, less luminous component appears connected, suggesting an ongoing interaction. There's a color gradient evident, with a central region appearing more yellow-red and potentially indicating an older stellar population or increased dust obscuration, while the outer regions show bluer hues, possibly related to recent star formation activity. The overall appearance suggests a galaxy with a considerable mass and a moderate star formation rate, currently experiencing gravitational interaction.