The galaxy presents as a disturbed system. It appears to be undergoing a significant interaction or merger event. The primary body exhibits a somewhat amorphous shape, deviating from a clear spiral or elliptical structure. There is a central concentration of light, suggesting a prominent nucleus or bulge region. Patches of bluer light are observed, indicative of ongoing star formation. Fainter reddish or orange hues are also seen, potentially associated with older stellar populations or regions obscured by dust. The overall morphology suggests a system in a state of flux, possibly due to gravitational interactions with another galaxy or internal dynamic processes. There is evidence of tidal features or debris extending from the main body, further supporting an interaction scenario.
