The galaxy appears to be undergoing a merger event. Two distinct components are visible, with a brighter, more diffuse region dominating the right side of the image and a slightly smaller, less luminous region visible to the left. Both components exhibit a generally smooth appearance, though there is some indication of tidal distortion or disturbance in the overall morphology.

The brighter component shows a greenish-white core, potentially indicating intense star formation activity or an active galactic nucleus. A reddish hue is noticeable in the central region, and the surrounding area shows a blue tinge.

The less luminous component shows a more concentrated central region with a reddish color, suggesting an older stellar population. There is also evidence of faint blue emission in the outer regions, possibly from younger stars.

The overall shape of the galaxy is irregular, further supporting the hypothesis of an ongoing or recent merger. The interaction between the two galaxies appears to have triggered star formation in both components, as indicated by the presence of blue light.
