This galaxy appears to be undergoing a merger. There are two distinct nuclei visible, both exhibiting a smooth, relatively featureless morphology. The northern nucleus is slightly more diffuse in appearance than the southern one. Faint tidal features or disturbances are not readily apparent in this image, suggesting that the merger is either in its early stages or that any tidal features are too faint to be detected with the available data. The overall color suggests an evolved stellar population, with a higher concentration of older, redder stars. The galaxy appears to be relatively round in shape, though the presence of a merger makes it difficult to determine an intrinsic shape. Based on the overall appearance, the galaxy shows some signs of weak or non-existent star formation activity. 
