The galaxy appears to be undergoing a significant merger event. There are two distinct components: a larger, yellowish, and relatively smooth structure and a smaller, bluer, and more diffuse structure. The larger component exhibits a concentrated central region, suggesting a more evolved stellar population. The bluer component displays a less defined structure, possibly indicating active star formation. Tidal features are not readily apparent, but the irregular shape of the combined system implies gravitational interaction. The overall morphology suggests a system that has experienced a recent or ongoing merger, disrupting its original form. The galaxy's light is primarily emitted at shorter wavelengths, suggesting that it consists of old stars. The lack of structure suggests that the galaxy is an elliptical galaxy.
