The galaxy presents an elongated, disturbed morphology, suggestive of an ongoing or recent interaction. The light is bluer at the center and at the top end of the galaxy, which could indicate regions of elevated star formation activity. The central area displays a higher concentration of luminosity, potentially indicating a galactic nucleus. There is a significant presence of disturbed features or tidal tails, supporting the hypothesis of a merging event. A higher proportion of the galaxy could have an edge-on disk. There is a presence of light in the redder part of the spectrum, suggesting an older stellar population.