This galaxy exhibits an elongated, somewhat irregular morphology. The main body of the galaxy appears relatively smooth but also shows significant disturbances or asymmetries in its overall structure. A concentration of light, potentially representing a galactic nucleus or a region of intense star formation, is observed in the center. Fainter, diffuse light extends outwards, creating a wispy, disturbed halo surrounding the main body, hinting at a possible ongoing or recent merger event. Patches of blue light are scattered through the halo, with a few notably brighter regions appearing as distinct knots, possibly indicative of star formation. The overall color appears relatively blue-white, suggesting a presence of young, hot stars, although there may be regions of older, redder stars. The shape, light distribution and features within the main body, coupled with the disturbed halo, indicate the galaxy is either in the midst of or recently underwent a merger event, resulting in structural and star-formation irregularities.
