This galaxy exhibits a morphology suggestive of an ongoing merger or significant gravitational interaction. The primary body of the galaxy displays a diffuse, somewhat amorphous structure, lacking a well-defined spiral or elliptical shape. There is an overall smooth appearance, though some irregular features are present, particularly in the form of extended tidal tails or distorted arm-like structures. A distinct bright core is observed, indicating a concentration of stars in the central region. Color variations across the galaxy suggest differing stellar populations and/or dust content. The blueish tones indicate the likely presence of young, hot stars, possibly formed through the merger event. The overall red color of the galaxy is apparent as well, indicating a later stage in galactic evolution.
