This galaxy presents as a disturbed spiral system. A central bulge is evident, with a bright, compact core indicating a possible active galactic nucleus. Faint spiral arms extend outward from the bulge, but they are somewhat disrupted and show signs of tidal interactions or past mergers. The galaxy's overall structure suggests a system undergoing a significant gravitational disturbance. Patches of blue light are visible within the arms, indicating regions of ongoing star formation. There are hints of dust lanes visible that obscure some portions of the galaxy. Overall, the galaxy's morphology suggests a system in transition, possibly recovering from a recent merger event.
