I suspect @Christoper James Huff's comment is right in that it doesn't really matter where the upper stage goes for this kind of high energy launch. The lyrics of Tom Lehrer come to mind here:
"Once the rockets are up,
Who cares where they come down?
That's not my department,"
Says Wernher von Braun
Additionally, looking at one of the referenced answers, there is the possibility that the Falcon 9 (v1.1 at the time) did not have enough "excess performance" to do a disposal burn. Using HORIZONS you can compute the launch C3 of TESS and DSCOVR (and DART for good measure):
| Spacecraft (Launcher) |
C3 (km^2/s^2): |
Mass (kg): |
| TESS (F9 B.4) |
-2.8 |
362 |
| DSCOVR (F9 v1.1) |
-0.6 |
570 |
| DART (F9 B.5) |
6.5 |
610 |
(all three missions performed a drone ship landing*, TESS did a disposal burn, DART did not have to: C3>0)
Noting that the jump from v1.1 to B.4 increased performance by ~33% (according to Wikipedia), it's plausible that the DSCOVR 2nd stage just didn't have anymore juice to perform a burn (and thus did not).
*SpaceX used the DSCOVR launch to test first stage recovery doing a soft ocean landing down range (no drone ship).
Bill Gray of Project Pluto has been tracking this object:
What was the timeline on figuring this out?
DSCOVR (and this rocket stage with it) passed close by the moon on
2015 February 13, not long after launch. About a month later, one of
the asteroid surveys found this object and posted it to the NEOCP
(Near-Earth Object Confirmation Page). This is where astronomers post
data about objects they've found that might be near-earth asteroids or
comets; the idea is that others can then try to observe them as well
and say "I found it, too, at the following location" or "Hmmm, can't
find that one." The discoverers, thinking they had a rock, gave it the
temporary name WE0913A.
In this case, a small observatory in California got more data,
followed by enough data over subsequent days that I could show that
WE0913A had made a close flyby of the moon on 2015 February 13.
Further checking confirmed that the flyby matched the one the DSCOVR
second stage would have made, and we abandoned the hope that it might
be a rock. (Asteroid people want to find asteroids; junk is a bitter
disappointment.)
The object's cis-lunar chaotic orbit is shown here since the start of 2022:

(Project Pluto)
With animations here and here.