The galaxy presents a complex morphology, possibly indicative of an ongoing or recent interaction. A dominant, relatively smooth and centrally concentrated component appears to be undergoing a merger with at least one smaller satellite galaxy. This primary galaxy exhibits a generally elliptical shape and a yellowish-orange hue, suggesting an older stellar population. Evidence of tidal disturbances is visible, with diffuse extensions of light extending from the main body. There is also a distinct, more compact and bluer region. Overall, the system appears to be a relatively massive object with moderate star formation activity.
