This galaxy exhibits a complex morphology, potentially indicative of a galaxy merger event. It has a central concentration of light, but not a singular nucleus; instead, it appears to have two distinct, bright, yellowish-orange cores separated by a small distance. These cores are embedded within a diffuse, surrounding halo of fainter, greenish light. The overall shape deviates significantly from a smooth, elliptical profile. There are hints of tidal tails or bridges extending from the main body, suggesting gravitational interactions. The galaxy's color suggests a mix of stellar populations with ongoing star formation. The light appears to be generally reddish, indicating that much of the stellar population is older. The greenish light may indicate a relatively young stellar population. This galaxy appears to be in a dynamic state, possibly undergoing a significant transformation due to the merger.
