The galaxy appears to be undergoing a merger event. There are two distinct, bright cores visible, suggesting two galactic nuclei in close proximity. The morphology is somewhat amorphous, lacking a clear spiral structure or elliptical shape, indicative of gravitational interaction disrupting the original galactic forms. The overall color of the system appears yellowish-orange, possibly indicating a population of older stars and a relatively low rate of on-going star formation. Some tidal features may be present, appearing as faint extensions or disturbances in the surrounding halo, but are not very pronounced. The system appears relatively compact.
