This galaxy exhibits a complex morphology, possibly indicative of an interaction or merger event. There appears to be a relatively smooth, round component, which could be a bulge. Adjacent to this is a more diffuse and potentially disturbed region, showing hints of tidal features or disrupted structure. There is a color gradient across the object, with bluer colors concentrated in the brighter regions, suggesting the presence of younger stellar populations and ongoing star formation. The redder regions are more extended, potentially representing older stellar populations. Overall, the galaxy appears to be undergoing significant evolutionary processes, with a mix of established and actively forming stellar populations. The faintness and fuzziness of the image indicate this object is very distant.
