This galaxy exhibits characteristics suggesting a disturbed morphology, possibly indicative of an interaction or merger. The central region appears relatively smooth and concentrated, but there are faint features extending outwards. A plume-like structure extends from the galaxy, indicating tidal interaction. Overall, the galaxy presents a slightly irregular form. Colors suggest a population of older stars but faint signs of more recent star formation, likely triggered by the interaction event. The apparent size indicates it is a substantial galaxy at significant cosmological distance.
