The galaxy appears to be a spiral galaxy, although its structure is significantly disrupted. The core is relatively bright and somewhat centrally located. Faint spiral arms extend outward from the core, but they are not well-defined or continuous. There is evidence of significant tidal disruption and possible ongoing merger activity. The arms appear warped and distorted, with irregular patches of bright star formation. One side of the galaxy appears more extended and shows more signs of disturbance than the other. There are hints of a faint tidal tail extending outward. Overall, this galaxy appears to be in a dynamic and possibly transitional state.
