The observed galaxy exhibits an irregular morphology, displaying characteristics suggestive of an ongoing or recent merger event. The central region presents a complex structure with enhanced blue emission, indicative of active star formation. This region is surrounded by a more diffuse, fainter halo. Two distinct tidal tails appear to emanate from the central body, extending in opposite directions. These tails display a patchy distribution of luminosity, potentially resulting from gravitational interactions. The overall color gradient suggests a higher concentration of older stellar populations towards the outer regions of the galaxy, excluding the tails. The galaxy lacks a well-defined nucleus or spiral arm structure, consistent with a system undergoing significant gravitational disturbance.
