The observed galaxy presents as an amorphous, irregular structure dominated by reddish hues in its core, transitioning to a bluer, diffuse halo. There is evidence suggesting recent or ongoing interaction. The core exhibits a bright central region which may be indicative of active galactic nuclei or intense star formation. There appears to be tidal features indicative of an advanced state of merging or interaction with a companion. The halo shows a faint, irregular extension. The overall morphology is suggestive of a system undergoing significant gravitational disturbance.
