Appears to be a star leaving a high mass or high opacity tail for approx 5 or more diameters behind it

https://decaps.legacysurvey.org//viewer/?ra=225.1497&dec=-63.2211&layer=decaps2&zoom=12

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Its a Herbig-Haro Object (Herbig–Haro object - Wikipedia). Very cool phenomena related to very young stars interacting with the gas/dust of the ISM.

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Thanks Tom, I’ll check it out.