The galaxy appears to be an interacting system, likely in the late stages of a merger. The morphology suggests two distinct nuclei, visible as enhanced regions of light. The primary component displays a largely smooth appearance, with a high degree of central concentration, while the second has an amorphous shape. There are no clear spiral arm structures or prominent dust lanes visible. The galaxy exhibits a reddish hue, potentially indicating an older stellar population, and the estimated redshift places this galaxy at a considerable distance. The overall interaction is indicative of tidal forces and gravitational disturbances reshaping the structure. Star formation is likely present, but the older stellar population masks more prominent blue colors.
