This galaxy appears to exhibit features indicative of a recent or ongoing merger event. The primary body is somewhat amorphous, lacking a well-defined spiral structure. The central region displays a brighter, more condensed concentration of light, with the light appearing to be primarily in the green portion of the spectrum. Extending from this central region are faint plumes or tidal tails. These structures suggest gravitational interaction with another galaxy. One of these tails stretches out noticeably farther than the other, with a reddish/orange hue at its end. The overall shape of the galaxy deviates from a classic elliptical or spiral form, suggesting a disrupted morphology. Further investigation is needed to determine the full extent of the merger and the properties of the interacting galaxies.
