The galaxy presents as a merging system. It appears to be comprised of two main bodies, both with a generally smooth morphology. The primary body shows a concentrated core region of yellowish-orange hue, indicative of an older stellar population and possibly dust extinction. A less defined and less concentrated secondary body is located adjacent to it. Faint tidal features extend outward, suggesting gravitational interaction. Some blue-ish emissions may indicate regions of lower density star formation. Overall, it suggests a galaxy merger in progress.
