The galaxy presents a distinctly non-smooth morphology, exhibiting characteristics indicative of a spiral structure. Spiral arms are clearly visible, with a predominant number exhibiting a two-armed configuration and a loose winding pattern. The presence of a bar feature appears to be moderate in strength. The bulge component is present but small to moderate in size relative to the disk. There are noticeable signs of interaction or disturbance affecting the galaxy's structure. The tidal tails indicate a possible ongoing merger. There seems to be a possible remnant of an older galaxy embedded in the current galaxy. It appears that a major disturbance may have caused this interaction. There are visible dust lanes across the galaxy disk. Star formation regions are suggested by blue hues.