The galaxy presents a diffuse morphology, appearing to be weakly structured. Its color is predominantly greenish, hinting at a possibly high star formation rate with corresponding emission lines. There is a notable lack of a defined nucleus, suggesting a relatively low central mass concentration, or that it is obscured by dust. Faint indications of a possible distorted tidal feature appear on the right side of the galaxy, suggesting a past interaction or merger event. There is no obvious spiral structure or bar feature. Overall, the galaxy appears to be a disturbed, irregular object.
