The galaxy presents as a spiral type, albeit with a somewhat disturbed morphology, potentially indicating ongoing or recent interaction with another galactic object. Its central bulge displays a moderate concentration of light, suggesting a developed but not overwhelmingly dominant structure. Diffuse spiral arms extend outward, exhibiting a blueish hue indicative of recent or ongoing star formation within these regions. There is evidence of asymmetrical features or tidal tails extending from the main galactic body, particularly on the left side of the image, strengthening the hypothesis of an interaction or merger. The overall color gradient shifts from a yellow/orange core to bluer outer regions, typical of galaxies experiencing active star formation in their spiral arms.
