The galaxy presents an elongated, somewhat cigar-shaped morphology. A noticeable color gradient is observed. A central, yellowish-orange concentration appears to dominate the core region. Moving outward, the galaxy transitions to a greenish-blue hue, particularly noticeable on one side, suggesting potential disk-like structures. The overall structure appears somewhat disturbed, but not dramatically so, hinting at a possible past interaction or minor merger event, or perhaps internal dynamic processes. There is a suggestion of underlying spiral arm-like features. The features appear to be moderately smooth.
