This galaxy exhibits a complex morphology, suggesting an ongoing or recent interaction. The primary body of the galaxy appears somewhat disk-like but with significant disturbances. There is a noticeable elongation in its overall shape, possibly indicating tidal forces at play. A brighter, more concentrated region is visible at its core, which likely hosts the galactic nucleus. Blue hues are present throughout the galaxy, especially in the outskirts, suggestive of active star formation regions. A fainter extension or tail-like feature is observed on one side of the galaxy, further supporting the likelihood of a merger event. The overall structure is not smoothly elliptical, indicating a system that is dynamically disturbed and undergoing significant changes.
