This galaxy appears to be an interacting pair, with two distinct components that are likely in the process of merging or at least gravitationally influencing each other. Each component presents a disk-like morphology, exhibiting a flattened structure. Both disks are oriented at an angle relative to our line of sight. They exhibit a primarily smooth texture with no obvious spiral arms, suggesting an earlier type or a disk that has been disrupted by the interaction. The overall color of the galaxy is yellowish-white, indicative of a population of older stars and a relatively low rate of ongoing star formation. There might be some evidence of tidal features or distortions in the outer regions of the galaxy, which further supports the interpretation of an ongoing interaction. The system appears relatively undisturbed beyond the immediate vicinity of the two main components.
