The galaxy presents as a dual-component system. A bright, relatively compact, blue-shifted core dominates the central region. This core is surrounded by a fainter, more diffuse structure. The core exhibits a near-spherical morphology. 

The secondary component appears as a flattened, disk-like structure oriented approximately edge-on relative to our line of sight. This disk component displays a reddish-yellow hue, contrasting with the blue core. There is some evidence of asymmetry or minor disturbances within the disk's structure, though a definitive classification of merging activity is unclear.
