The galaxy exhibits a morphology suggestive of an ongoing or recent merger event. The primary body of the galaxy displays a bright, concentrated core, indicating a significant population of stars in that region. Faint, diffuse emissions extend away from the main body, which is consistent with tidal tails resulting from gravitational interactions. The system lacks a defined spiral arm structure, instead showing irregular patterns of light distribution, with a color gradient, appearing bluer in certain areas, potentially indicative of more active star formation. Overall, the galaxy displays a disturbed and asymmetrical shape.
