This galaxy appears to be undergoing a significant interaction or merger. Two distinct components are readily observable. One component presents as an elongated, somewhat diffuse structure. It exhibits a smooth appearance, although subtle irregularities in brightness distribution may be present. The second component is more compact and concentrated, appearing nearly spherical. There may be some tidal distortion or stream present at the area where the two components are interacting. The overall color suggests a population of intermediate to old stars, with faint hints of blue indicating possible regions of recent star formation. Dust lanes or prominent spiral arm features are not clearly discernible, which is indicative of a smooth galaxy.
