The galaxy presents as a system likely undergoing a merger or significant tidal interaction. There are two distinct components. One component exhibits a smoother, more concentrated morphology, appearing spheroidal in shape. Its color is skewed towards the red end of the spectrum. The second component is more diffuse and elongated, with noticeable features that may indicate a disk structure, though heavily distorted. This component displays a bluer color, hinting at active star formation. The overall system has a disturbed appearance, suggesting gravitational interaction between the two galaxies. Some indications of tidal tails or bridges may be visible, linking the two components, though the image resolution limits detailed analysis of these features. Overall, the observed features suggest a galactic system in a relatively late stage of merging, with possible on-going star formation.
