The galaxy appears to be undergoing a merging event. The primary galaxy exhibits a flattened, disk-like morphology, with a noticeable bulge component that appears relatively smooth and centrally concentrated. There is a secondary, smaller object in close proximity. Both components show signs of tidal disturbances, indicated by faint and diffuse extended features. The colour of the galaxy appears reddish, suggesting an older stellar population and a relatively low rate of current star formation. Given the observed disturbances and close proximity of the two objects, tidal interactions are likely influencing the morphology of the system. The system appears to be relatively massive based on its overall luminosity.
