This galaxy appears to be undergoing a significant interaction or merger. The morphology is disturbed, with clear signs of tidal features or distortions in the galactic structure. It exhibits a generally elliptical form, but the shape is irregular and asymmetric. There appear to be two major components or nuclei, suggesting a possible ongoing merger event between two galaxies of dissimilar size.

The galaxy displays a mix of colors, with regions of bluer light indicating areas of ongoing star formation. Other regions exhibit redder hues, possibly indicating older stellar populations or dust obscuration.

The star formation rate appears relatively low, but not negligible. The specific star formation rate suggests a moderate level of activity compared to the galaxy's estimated stellar mass.

It seems that major disturbances are affecting the structure and dynamics of this system.
