The object presents as a galaxy at a moderate redshift, appearing as a somewhat diffuse, luminous structure. It appears to be composed primarily of older stellar populations as indicated by the redder colors. It shows a complex morphology that is not completely smooth. There are multiple distinct, bright knots of emission within the main body, potentially indicative of ongoing or recent merger activity. There may be minor disturbances within the central core as well. The overall shape approximates a slightly elongated spheroid.
