This galaxy exhibits a complex morphology, appearing to be in a state of interaction or merging. The overall form is somewhat irregular. There appear to be at least two distinct luminous components, possibly representing the cores of the interacting galaxies. One component displays a yellowish hue, suggesting a population of older stars. The second component has a bluer color profile, potentially indicating more recent star formation activity. There is faint, extended emission connecting the two central components, though it is unclear if this is the result of tidal interaction or the original structure of either system. There may be evidence of tidal tails or disrupted spiral arms extending away from the main body of the system, although this is difficult to confirm given the image resolution and the level of disruption to the galaxy's form. It seems as though it's in between a smooth and disk shape, slightly more smooth than disk. It looks like it is in the middle of a major merger.
