The galaxy appears to be undergoing a significant interaction or merger. The primary body displays a somewhat amorphous structure. A secondary component is visible, possibly indicating a recent or ongoing merger event. There is some evidence of tidal features or distortions suggesting gravitational interaction. The galaxy exhibits a relatively smooth overall morphology, potentially indicating an elliptical or lenticular classification, although the disturbance complicates definitive classification. The color profile suggests a population of older stars, with a moderate contribution from younger stars or ongoing star formation. The object does not appear to be a classic spiral or barred spiral galaxy, but its morphology is certainly peculiar due to the interaction.
