The galaxy exhibits a complex morphology, appearing to be in a state of interaction or merger. There is a distinct, brighter core region, possibly indicating a concentration of older stars or an active galactic nucleus. Emanating from this core is a fainter, more diffuse structure, suggesting tidal arms or disrupted material due to gravitational interaction. The color gradient is notable, shifting from a redder hue in the central region to a bluer tint in the outer arms or structures. This could indicate differing stellar populations or dust content throughout the galaxy. There appears to be significant disruption to the overall structure of the galaxy, rather than a symmetrical, elliptical, or spiral nature.
