The galaxy presents a somewhat disturbed morphology, suggesting ongoing interactions or recent merger events. Its overall structure exhibits both smooth and featured components. A central, brighter region indicates a higher concentration of older stars, potentially a bulge. Extending outward from the central region are fainter, irregular arms or features exhibiting a bluer hue, indicative of ongoing star formation. The disk, if present, shows no clear spiral structure, perhaps due to the interactions or merger events. Patches of enhanced blue emission are visible within the arms, likely regions of active star formation. The galaxy's light profile appears relatively compact, with the bulk of its luminosity concentrated in the central regions, tapering off into a faint halo or extended disk.
