The observed galaxy appears to exhibit a complex morphology, with notable features suggesting possible interactions or internal disturbances. The overall structure lacks a clear, defined shape, implying a potentially irregular or transitional state. Patches of nebulosity are visible, particularly in the central and lower regions, exhibiting variations in intensity and color. These nebulae could represent areas of active star formation. Faint, extended features hint at tidal arms or debris trails, pointing toward possible past or ongoing interactions with another galaxy. The general structure of the galaxy indicates a disturbed system. The core may be present but it is heavily obscured by gas. Evidence of mergers or other galactic interactions is visible in the form of distorted structures within the galaxy.
