The galaxy presents with an ambiguous morphology. It has a dual structure, with a brighter, rounder component positioned above a slightly elongated, fainter component. The upper component exhibits a yellow-gold hue and appears relatively featureless, suggestive of an elliptical or lenticular morphology dominated by older stellar populations. The lower component presents a bluer hue and hints at a disk-like structure, potentially indicative of ongoing star formation, although this is not definitive from the image alone. The two components are in close proximity and appear gravitationally interacting, with some possible tidal distortion or disturbance. There may be a faint tidal tail or bridge of material extending between the two components. While the rounder component appears more homogenous, the lower, bluer component shows hints of internal structure, perhaps spiral arms or dust lanes. Further spectroscopic data is required to properly assess the redshift and star formation.
