This galaxy exhibits a morphology suggesting an ongoing merger event. Two distinct luminous regions are apparent, one with a bluer spectral signature and the other with a redder spectral signature. The bluer region suggests a higher proportion of younger, hotter stars, while the redder region implies an older stellar population. The overall shape of the galaxy lacks a clear spiral or elliptical structure; instead, it appears distorted and irregular, indicative of gravitational interactions. The presence of tidal tails or bridges is not definitively apparent in the provided image, though some faint extensions are visible. The relative sizes of the two luminous regions are roughly comparable. 
