This galaxy exhibits a disturbed morphology, possibly undergoing a merger event or experiencing tidal interactions. It presents an elongated shape, not perfectly elliptical, indicating a deviation from a relaxed state. The light distribution shows distinct clumps or knots within the galactic structure, suggesting regions of enhanced star formation or remnants of the interacting galaxies. The color gradient indicates a varying stellar population, with the central region appearing relatively redder, potentially signifying older stars or dust obscuration, while the outer regions seem bluer, hinting at the presence of younger, hotter stars. There may be evidence of a faint tidal tail or bridge extending from the main galactic body, although this is difficult to ascertain due to image resolution. Overall, the galaxy appears to be a dynamic system that is evolving as a result of external influences.
