This galaxy exhibits a morphology characterized by significant disturbances, potentially indicative of an ongoing or recent merger event. The overall form is somewhat amorphous, lacking a well-defined spiral or elliptical structure. The light distribution appears complex, with several brighter regions suggesting localized star formation or tidal features resulting from the interaction. The galaxy's color profile suggests the presence of both older stellar populations and younger, bluer stars, which is consistent with the disturbance observed in the morphology. The general appearance of the galaxy suggests a dynamic system with ongoing or recent star formation activity influenced by gravitational interactions.
