The galaxy appears to be a spiral galaxy with a redshift of approximately 0.24. The morphology suggests a possible ongoing or recent interaction or merger, evidenced by tidal disturbances or asymmetries in the outer regions. The galaxy is observed to be moderately blue, indicative of some ongoing star formation, but with a considerable presence of older stellar populations. The galaxy exhibits no obvious distinct central bulge. There seems to be patchy extinction. Overall the image suggests a mid-mass galaxy undergoing or recently having undergone some kind of disruptive event.
