The galaxy presents as a merging system composed of two primary components. The larger, more diffuse component appears yellowish, suggesting a population of older stars and/or significant dust obscuration. Its shape is roughly elliptical, but shows some signs of tidal distortion. The second component is more compact and exhibits a reddish hue, potentially indicating a region of intense star formation heavily embedded in dust, or a population of very old stars. There are slight visual disturbances and asymmetries in the galactic structure, which is a characteristic feature of galaxies undergoing merging events. A high degree of morphological disturbance is visible, implying ongoing gravitational interaction between the two components. The general smoothness of the system, apart from the central merging region, indicates that this galaxy is a merging system which may evolve into an elliptical galaxy.
