The galaxy appears to be in a late-stage merger, exhibiting a highly disturbed morphology. Two distinct luminous components are visible. The primary component is relatively smooth and elliptical in shape, exhibiting a concentrated brightness profile. The secondary component is less distinct and appears more compact. There's an indication of tidal tails or other disruption signatures, pointing to gravitational interactions between the galaxies. There is a suggestion of ongoing star formation based on the slightly bluer color. Overall, the system exhibits characteristics of a dynamically active environment with ongoing or recent merger activity.
