The galaxy appears to be a spiral galaxy, likely seen at a shallow angle. One side of the galaxy exhibits a concentrated, bright, and relatively smooth disk or bulge. The color is yellowish, indicating an older stellar population. The opposite side shows a bluer and more diffuse region, indicating a region of active star formation, potentially an outer spiral arm or tidal feature. The overall morphology is somewhat irregular, suggesting possible past interaction with another galaxy or some internal disturbance.
