The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction or merger. A prominent, relatively smooth, and more luminous component is observed, appearing yellowish-orange in color. Adjacent to this is a fainter component, displaying a distinct blue hue, suggestive of active star formation. This blue region appears somewhat disk-like. There are indications of tidal features, perhaps faint tails or bridges, extending from both the brighter and the bluer component, although they are not well-defined. The overall structure suggests a non-equilibrium state, deviating significantly from a simple elliptical or spiral morphology. Further spectroscopic analysis would be necessary to confirm the presence of tidal features and assess the age and metallicity of the stellar populations within each component, helping constrain the galaxy's formation history.
