The galaxy appears to be undergoing a merger, displaying a complex morphology suggesting gravitational interaction. It exhibits a relatively smooth, centrally concentrated component with an overall elliptical shape, indicating a substantial spheroidal population.

One of the merging components displays a distinctly yellowish-white color, implying a population of older stars. The second component presents a more reddish-orange hue, potentially due to the presence of dust and younger, actively star-forming regions. The relative distribution of light suggests a high luminosity.
