This galaxy presents as a disturbed system, possibly undergoing a minor or major interaction with a second, smaller galaxy. The primary galaxy exhibits an elongated, cigar-shaped morphology, indicating it is likely an elliptical or lenticular galaxy, but the disk appears to have been warped due to the interaction. There is a significant amount of diffuse light surrounding the central region, suggestive of tidal features. The color gradient indicates a higher concentration of older stars. This galaxy exhibits a moderate estimated redshift of 0.215631. This value corresponds to an approximate lookback time of 2.68 billion years. Finally, the current estimated star formation rate is approximately 10^1.8293 to 10^1.9671 solar masses per year.
