The galaxy appears to be undergoing a significant merger event. Its morphology is highly disturbed, with a bright, somewhat amorphous central region. There are at least two distinct nuclei visible, one appearing slightly more diffuse than the other, indicative of two galaxies in the process of coalescing. The overall color of the galaxy leans toward the redder end of the spectrum, suggesting a population of older stars, although some regions exhibit slightly bluer hues, potentially indicating pockets of ongoing or recent star formation. The galaxy lacks a clear spiral arm structure or a well-defined disk, further supporting the classification as a merging system. Tidal features, such as extended tails or bridges of stars and gas, are not immediately apparent, however, this could be due to the resolution or depth of the image.
