The galaxy presents as a dual system, possibly interacting, and is observed at a redshift suggesting a considerable distance. One component appears as a relatively smooth, elliptical galaxy with a concentrated central region, emitting a yellowish-white light suggesting an older stellar population with suppressed star formation. The second component shows a disturbed morphology, exhibiting a bluer hue indicative of ongoing star formation. Faint tidal features may be present, extending from the disturbed galaxy, possibly indicating a gravitational interaction between the two galaxies. There is evidence of dust lanes and irregular structure within the bluer component. A merger is probable based on the asymmetric shape and disturbed features.
