The galaxy presents a morphology suggestive of an ongoing or recent merger. It appears to consist of two distinct components: a more centrally condensed, yellowish-white region, and a less concentrated, bluer region adjacent to it. The yellow-white component could represent the remnant core of one of the progenitor galaxies, likely composed of an older stellar population. The bluer component exhibits a more diffuse structure, possibly indicative of enhanced star formation activity, which is a common consequence of galactic mergers. Tidal features or distortions are not readily apparent in this image, but this could be due to limited image resolution or the advanced stage of the merger. The system exhibits an overall apparent smoothness, although there is some indication of irregular structure within the fainter, blue-dominated region.
