The galaxy exhibits a disturbed morphology, potentially indicative of a merger or interaction. There is evidence of multiple distinct components or nuclei. One component displays a reddish-yellow color, suggesting an older stellar population or dust obscuration. Another component presents a bluer hue, implying younger, hotter stars and ongoing star formation. There are faint tidal tails or streams of material extending outwards from the galaxy, further supporting a past or ongoing interaction. The galaxy's overall structure does not conform to a regular elliptical or spiral shape.
