This galaxy appears to be undergoing a major merger. There are two distinct nuclei visible. The larger of the two nuclei exhibits a diffuse yellowish-orange glow, indicative of an older stellar population. The second, smaller nucleus is also yellowish-orange, and appears to be slightly more compact.

Tidal features are evident around both nuclei, suggesting strong gravitational interactions. There is some evidence of irregular, faint extensions or tails emanating from the system, furthering the indications of a disruptive merger event. The overall color profile suggests a population that is relatively quiescent, with limited active star formation.
