The galaxy appears to be undergoing a significant interaction or merger. The primary morphology is highly disturbed, displaying a non-smooth structure with evidence of tidal features and distortions. Two distinct, brighter components are visible, suggesting the presence of two interacting galactic nuclei. A faint bridge of material connects these two brighter regions, indicating gravitational interaction and potential mass transfer. The color gradient within the galaxy suggests differential stellar populations or varying levels of dust extinction across the system. The overall color is a slightly yellow hue. There are signs of possible star formation activity within the regions of higher density. There seems to be several tidal tails originating from this disturbed galaxy.
