This galaxy appears to be undergoing a significant interaction, possibly a merger. Two distinct nuclei are visible within a common, diffuse halo of light. The overall color is reddish-yellow, suggesting an older stellar population and relatively little ongoing star formation. The shape is irregular, lacking a well-defined spiral or elliptical structure, further indicating a disturbed morphology likely due to the gravitational interaction. There is evidence of faint tidal features extending from the main body of the galaxy, hinting at the scale of the gravitational disruption. While appearing relatively smooth in the central regions, the outer regions exhibit a more disturbed and complex structure. The overall system is compact in size.
