The galaxy presents as a dual-core system, potentially indicative of an ongoing or recent merger event. The larger, primary core exhibits a smoother, more diffuse appearance, with a color gradient shifting from a central, bluish-white hue to a yellowish-white periphery. The secondary core appears more compact and possesses a distinctly warmer, yellowish-orange color. Faint tidal features or stellar streams may be present, but the image resolution limits definitive confirmation. The overall morphology suggests an elliptical-like structure, though disturbances could be obscuring underlying disk features. A fraction of the object appears as an artifact. Further spectroscopic analysis would be valuable to determine the redshift, metallicity, and star formation rate within each core.
