The galaxy appears to be in a state of interaction or disturbance, exhibiting an irregular morphology. It displays a somewhat diffuse central region with what looks to be a few prominent, bright knots of light. Faint tidal features or plumes extend outwards. The color gradient suggests a possible mixture of older stellar populations. The galaxy is quite large. There may be an ongoing merger event. The structure may be a disk galaxy, but this is difficult to confirm given the disturbances. There seems to be evidence of active star formation.
