The galaxy presents as an elongated structure, suggestive of a disk galaxy viewed at a significant inclination. Its color profile indicates a gradient, transitioning from a bluer hue towards one end to a redder, yellower tone at the opposite extremity. This color difference could imply varying stellar populations and dust content within the galaxy, with the bluer regions potentially harboring younger, hotter stars and lower dust extinction compared to the redder regions. The light distribution seems relatively smooth across the galaxy's body with some evidence of clumpiness. Overall, the galaxy's morphology suggests a relatively evolved system potentially undergoing active star formation in some regions, as the object also has properties of being a merger.
