The galaxy appears to be part of a binary system, possibly a galaxy merger or a close interacting pair. Each component exhibits a relatively compact morphology, with a bright, concentrated core. The light distribution suggests a degree of smoothness, though some irregular features and disturbances are present. A slightly asymmetric shape is also visible. The color of the galaxy is a pale blue-white, indicating a moderate amount of star formation. Further analysis is needed to determine the extent and nature of the interaction, as well as the individual properties of each component galaxy.
