The galaxy appears as a centrally concentrated object with a generally smooth morphology. There are two prominent, partially overlapping light sources, suggesting a possible recent or ongoing merger event. The galaxy's shape is roughly circular with minimal elongation. Color analysis indicates a redder component and yellower component with the yellower area seeming to dominate the galaxy's overall light output, which implies active star formation. There are minor signs of tidal disturbances within the image, indicating gravitational interactions. The galaxy appears to be relatively massive, likely indicating it is a mature system. Based on its inferred low star formation rate, the galaxy may be transitioning towards quiescence. 
