The galaxy appears to be a luminous object at a considerable redshift. It exhibits a somewhat irregular morphology, possibly undergoing some form of interaction or disturbance. There is a notable central bulge region with a yellowish hue. This may indicate an older stellar population, possibly with reduced rates of active star formation. Fainter, somewhat diffuse extensions are also present, displaying a bluer color suggestive of the presence of younger, hotter stars and regions of active star formation. There appear to be disturbances to the galaxy's overall structure. This could indicate an ongoing merger or interaction with another galaxy. This disturbance is causing asymmetrical light profiles throughout the galaxy, suggesting tidal features or warped stellar distributions.
