The galaxy appears to be undergoing a merger, presenting a disturbed morphology. Two distinct, bright nuclei are visible within the galaxy's overall structure, suggesting the interaction of two galaxies of potentially similar sizes. The system exhibits an elliptical shape overall, with diffuse, faint outer regions surrounding the brighter central areas. There is a suggestion of tidal features or extended plumes extending outwards. These faint features indicate gravitational disruption. Color gradients are subtle, with the nuclei exhibiting a slightly yellower hue, potentially indicating an older stellar population. The outer regions appear slightly bluer. This galaxy seems to be relatively massive, with intermediate star-formation. The system is not strongly star-forming and is not actively creating stars.
