This galaxy appears to be undergoing a significant interaction, possibly a merger. The morphology is complex, showing signs of tidal disruption and disturbed structure. There are two main luminous components. One component exhibits a smoother, more concentrated appearance, likely representing the remnant core of one of the original galaxies. Its color is skewed toward the redder end of the spectrum. The second component, appearing to the left, has a bluer hue. This suggests a region of active star formation possibly triggered by the interaction. Faint tidal tails or streams are potentially present, extending from the main body. The overall shape deviates considerably from a regular elliptical or spiral. The system appears to be relatively compact. The galaxy is not a pure disk but appears to have a complex internal structure.
